The galaxy presents as a fairly elliptical structure, with a significant central bulge that displays a yellowish hue, potentially indicating an older stellar population. The outer regions appear bluer, suggesting the presence of younger, hotter stars and perhaps some ongoing star formation, though not dramatically so. There is a slight flattening visible, suggesting the galaxy may have a disk component, but the bulge dominates the overall morphology. The galaxy appears relatively smooth in texture, lacking any obvious spiral arm structures or significant dust lanes. There is a subtle asymmetry, with one side appearing slightly more extended or disturbed than the other, which may imply minor gravitational interactions or tidal disturbances, although no clear companion galaxies are immediately evident. The light profile seems to follow a fairly concentrated Sersic profile, with a gradual fall-off in intensity from the center outwards.
