I will only make an answer about the position operator.
The most well-defined things that we may reliably say that we can measure, are Hamiltonian eigenvalues. It should be good on hindsight---you can keep measuring in succession, over a region of time, and keep getting the same value. This is the most certain we may become of anything in quantum theory.
This means that, really, momentum eigenstates are more fundamentally understandable than position eigenstates, because at least the free particle Hamiltonian, or the asymptotically free states of interacting Hamiltonians, corresponds to momentum eigenstates. Position representations are really just for us to make sure that we write down spacetime localised field interactions. (Remember that, as long as we want the field commutators to vanish for ``macroscopically space-like", meaning that fields do not interact with each other if they are sufficiently far apart, then they must also vanish microscopically. The proof of this is in "PCT, Spin and Statistics, and All That".)
The offending reason why position eigenstates are non-relativistic, is that
$$
\hat\phi_{\text{NR}}(\vec x,t)=\int\frac{\mathrm d^3p}{(2\pi)^3}\hat{\tilde\phi}(\vec p,t)e^{i\vec p\cdot\vec x}
\qquad \text{but} \qquad
\hat\phi_{\text{SR}}(\vec x,t)=\int\frac{\mathrm d^3p}{(2\pi)^32E_p}\hat{\tilde\phi}(\vec p,t)e^{i\vec p\cdot\vec x}
$$
notice that it is just a $2E_p$ in the denominator that is all the difference. The non-relativistic field has a sensible interpretation as a probability amplitude in the position representation, but it is manifestly non-relativistic because $\hat{\tilde\phi}(\vec p,t)e^{i\vec p\cdot\vec x}$ is manifestly relativistically invariant while $\frac{\mathrm d^3p}{(2\pi)^3}$ is missing the $2E_p$ in the denominator away from being relativistically invariant. This is contrasted with the relativistic version, which is manifestly relativistically invariant but has no nice interpretation as a probability amplitude in the position representation.
This is also why you will not find QFT authors discussing position representation of wavefunctions. They know this is a pain point. It is not just for massless particles; it affects massive particles too, but for the case of massless particles, it is particularly bad, because then we cannot pretend that there would be a sensible $2E_p\to2m_0c^2$ region, which can then be extracted out of the integral as a constant, and thus approximately considered as a position representation probability amplitude.