The galaxy presents a mostly smooth morphology, suggesting a relatively evolved system. It appears elliptical in shape, deviating slightly from perfect circularity. The central region exhibits a bright, concentrated bulge, which gradually fades into a more diffuse halo.

The color profile indicates a dominant older stellar population, with a yellow-red hue across the galaxy. There is a subtle hint of bluer regions in the outer disk or halo, potentially indicating some ongoing, although low level, star formation. Overall, the galaxy appears quiescent in terms of star formation activity. There is no obvious indication of tidal features or major mergers, suggesting that it has been undisturbed for a significant period of time.
