This galaxy appears as a relatively smooth, elliptical-like structure with a concentrated central bulge. It has a fairly round appearance, exhibiting some features but without a distinct disk or spiral arms easily discernible at this resolution. The light is primarily bluish-white, which could indicate the presence of younger, hotter stars. The galaxy displays no obvious signs of major ongoing mergers, though some minor disturbances might be present. The mass suggests this is a modest-sized galaxy. Given the color and apparent smoothness, the star formation rate seems comparatively low.
