coincidence? I don't think so!

There are two mechanisms relevant for baryonic feedback in galaxy formation: Supernova-feedback at low halo masses and AGN-feedback for high halo masses, and one obtains the least efficient feedback (or the highest retention of baryons) at around \(10^{12}M_\odot/h\), i.e. exactly the mass of our Milky Way. Is this a coincidence? Or could one set up an anthropic argument that we as observers are particularly likely to be in a galaxy with the lowest possible baryonic feedback?