The galaxy appears to be a relatively smooth, elliptical-type galaxy. It exhibits a concentrated, bright central bulge that gradually fades into a less defined halo. The overall shape is largely spheroidal, with minimal indication of a disk or spiral structure. There are no obvious signs of recent major mergers or tidal disturbances in the immediate vicinity of the galaxy. The light distribution is fairly uniform, suggesting an older stellar population with ongoing, low-level star formation, particularly based on its color.
