The galaxy appears as a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge, characterized by a slightly redder hue, transitioning into a bluer, more diffuse halo. There appears to be little indication of spiral arm structure, and it does not show signs of major morphological disturbances or ongoing major mergers, though some minor disturbances can't be ruled out. The overall roundness and lack of a distinct disk-like feature suggest a system dominated by an older stellar population, with a modest amount of ongoing star formation.
