The galaxy appears to be a relatively smooth, elliptical galaxy. It exhibits a concentrated central bulge that gradually fades into a diffuse halo. There is no apparent dust lane or spiral arm structure. The galaxy has an overall yellowish hue, which is most concentrated at the center, suggesting an older stellar population. The outer regions appear slightly bluer, potentially indicating some ongoing or recent star formation, although at a low rate. The galaxy's round shape indicates it is unlikely to be undergoing any major mergers or tidal disturbances. There are no visible signs of strong tidal tails or other indicators of significant interaction with nearby galaxies.
