The interaction mediated by a massive boson will produce interaction potential of Yukawa type:
$$
V(r) = - \frac{\alpha_\chi}{r} e^{-mr},
$$
As is well known, a scalar exchange leads to a universally attractive potential, whereas a
vector exchange will attract particles to antiparticles, but repel pairs of particles or pairs of antiparticles. For Z-boson eхchange $\alpha_\chi=g^2/4\pi$, $g$ is gauge coupling constant.
The existence of the bound states of two particles of mass $M$ in this potential (assuming $\alpha_\chi>0$) could be established in term of 'Bohr radius' $a$:
$$
a^{-1} = \frac {\alpha_\chi M}{2}
$$
Comparing this radius with the range of interaction $m$ yields dimensionless parameter:
$$
D =\frac{1}{am} = \frac {\alpha_\chi M}{2 m}.
$$
In order to have a bound state at all (the 1$s$ state), the potential must satisfy $D \gtrsim 0.8 $. So for a bound state through a weak force mass of the particle should be comparable (or greater) than mass of weak boson.
So for neutrino (or neutino + lepton) the mass $M$ is too small to allow any bound states.
However, various extensions to Standard model consider the possibility of additional weakly interacting massive particles: WIMP's, with masses much greater than that of neutrino, and which could constitute (part of) dark matter. So this particles potentially could form bound states based on weak force: WIMP-onium.
This states has been considered in literature. Take for instance paper:
Shepherd, William, Tim MP Tait, and Gabrijela Zaharijas. "Bound states of weakly interacting dark matter." Physical Review D 79.5 (2009): 055022. arXiv:0901.2125.
From the abstract:
We explore the possibility that weakly interacting dark matter can form bound states—WIMPonium. Such states are expected in a wide class of models of particle dark matter, including some limits of the minimal supersymmetric standard model. We examine the conditions under which we expect bound states to occur and use analogues of nonrelativistic QCD applied to heavy quarkonia to provide estimates for their properties, including couplings to the standard model. We further find that it may be possible to produce WIMPonium at the LHC and explore the properties of the WIMP that can be inferred from measurements of the WIMPonium states.