The answer from Nihar Karve provides useful information on how to describe spacetime in string theory, and I would like to add another perspective.
Closed string field theory describes spacetime curvature in (almost – see below) the same way as general relativity.
In general relativity, the dynamics of the metric $g_{\mu\nu}$ and the curvature of spacetime is described by the Einstein-Hilbert action coupled to some matter. And as you know, Einstein equation shows that the matter affects the curvature through its energy-momentum tensor. At this stage, there is no fixed background to describe GR, the fields do not propagate on something. In general, one looks to classical solutions to the equations of motion and start to study the properties of this specific spacetime and study how fields propagate on it.
Since it can be confusing to not have a background, a solution is to expand the metric around a fixed metric as $g_{\mu\nu} = \hat g_{\mu\nu} + h_{\mu\nu}$, where $\hat g_{\mu\nu}$ is fixed (and may or may not be a solution to the eom) and $h_{\mu\nu}$ is the new dynamical variable. Since the action is non-polynomial in $h_{\mu\nu}$, the simpler is to expand it in $h_{\mu\nu}$: you will get an infinite number of monomial interactions. As long as you keep all powers of $h_{\mu\nu}$, the action is completely equivalent to the original one (although it is now perturbative). The background is just a convenient computational tool, but it does not determine what is the physical spacetime. A nice example can be found in arxiv:2010.08882 where the Schwarzschild metric is recovered from amplitudes.
Closed strings unify both as matter and gravitons, so it is not possible to split them as we do in GR. However, it is possible to introduce an energy-momentum pseudotensor for gravity such that Einstein equations can be reformulated as a conservation law for the total matter+gravity energy-momentum tensor. This shows that there is no strong dichotomy between
Closed string field theory (SFT) provides an action for the string field, which is more conveniently studied in momentum space where you can see all the modes, including the graviton. In the latter form, the classical action just looks like GR expanded around a background (as described above).
For the free action of massless fields with general gauge fixing conditions, see arxiv:1206.3901. Everything you can do in GR, you can theoretically do it in SFT. The metric is split as $g_{\mu\nu} = \hat g_{\mu\nu} + h_{\mu\nu}$, so it is perturbative, but SFT itself tells you how to compute the action up to any power of $h_{\mu\nu}$ and you can also resum expressions (like in GR).
The only (technical) limitation is that you are basically forced to start with Minkowski as a background, $\hat g_{\mu\nu} = \eta_{\mu\nu}$.
(And obviously I am not saying that it is easy to do it in practice, just that it is possible in theory.)
Let me note stress that you don't need a background-independent nor non-perturbative formulation to already extract a lot of information.
To summarize, if the question is how to describe spacetime curvature in SFT, you just do what you do in GR expanded around a background. More generally, SFT is very useful and intuitive because you can see it as a standard QFT and use traditional methods (just being careful with the non-locality of interactions). The drawback is that it's not really teaching anything philosophical on spacetime.
(Let me note that it is my personal point of view: I don't any reference describing this, so maybe it's naive and other researchers may not agree.)