The galaxy appears to be a relatively smooth, elliptical-like structure. There is a concentrated central bulge. The galaxy displays a color gradient, appearing more yellow/white toward its core, suggesting an older stellar population. The outer regions exhibit a slightly bluer tint, hinting at the presence of some younger stars or ongoing star formation, albeit at a low rate. The overall form is somewhat flattened, and the light distribution smoothly decreases outwards from the center. There is no clear evidence of spiral arms or significant dust lanes within the resolution of this image. Close inspection does not reveal any signs of significant tidal disturbances or ongoing major merging events.
