We report on further observations of the luminous halo of NGC 5907. Ne
w V, I and B deep photometry confirms the existence of an extended ste
llar halo redder than the disk. Our data are consistent with a faint h
alo, or very thick disk, composed of a metal-rich old stellar populati
on. We propose that it could be the remnant of a merged small elliptic
al, and we support our hypothesis with N-body simulations.