The issue with harnessing the neutrino-electron interaction is the cross-sections involved. Since neutrinos are charge-less, and interact only via the weak force (gravity also but that won't help us here), they are more likely to interact with larger particles. For this reason, neutrinos-nuclei interactions are the most common.
While neutrinos can (and do interact) with electrons, they will likely encounter a much higher number of nucleons first. Here you can find some standard information on the neutrino scattering cross-sections. Note that the lowest nucleon-neutrino cross-sections will be three or more orders of magnitude larger than the electron-neutrino cross-sections.
Electrons don't like to be grouped together (both the electrostatic force and degeneracy pressure will push them apart) so to get a high enough concentration of electrons so that you'll be more likely to have e-$\nu$ interactions will be difficult. To compound this, high enough concentrations of neutrinos, to warrant enough interactions per second to result in energies required for propulsion, cannot be found anywhere except near supernovas and if you're near those, propulsion will be the least of your worries.
For comparison, on the Earth, the highest concentration of neutrinos come from the sun, which is estimated to produce neutrino flux on the order of ~ $10^{11}/cm^{2} s$ (source), whereas the interaction probability for a 1 MeV neutrino is on the order of ~ $10^{-11}$, for interacting with anything in the Earth as it passes through (source).