The galaxy appears to be a relatively smooth, elliptical galaxy. It exhibits a centrally concentrated luminosity profile, with a bright nucleus that gradually fades into a more diffuse halo. The galaxy has a generally rounded shape, with minimal evidence of strong spiral arms or significant disk structure. There may be a slight hint of a disk structure or a ring of material around the bulge, but the galaxy looks primarily elliptical in shape. There are no obvious signs of recent major merger activity or tidal disturbances within the main body of the galaxy. The color index suggests the stellar population is relatively old and dominated by evolved stars, and the weak star formation rate suggests the star formation activity has slowed considerably.
