The galaxy presents as an elliptical morphology, with a smooth, concentrated light profile. The central region is a bright, dense core that gradually fades into a more diffuse halo. There is a slight elongation, but the galaxy largely retains a rounded appearance. The color gradient suggests a population of older stars dominate the light output. There is little evidence of spiral arms or dust lanes. Tidal features are not discernible. There are some disturbances, however it appears as though a merger event is unlikely. The galaxy's moderate redshift suggests a considerable distance.
