The galaxy presents as a smooth, elliptical-like object with a concentrated central bulge. The light distribution exhibits a significant radial gradient, with the core region displaying a noticeably brighter and yellower color compared to the outer regions. This suggests an older stellar population dominating the central area. The outer regions appear more diffuse and slightly bluer, hinting at the presence of some younger stars or ongoing, albeit subdued, star formation activity. The overall shape is elongated, leaning towards an intermediate ellipticity. There is no clear evidence of spiral arms, a distinct disk, or prominent dust lanes. There is no strong visual evidence of any major ongoing mergers or tidal disturbances, although a very faint nearby source can be seen at the edge of the galaxy. This galaxy is likely a massive system with a relatively low specific star formation rate.
