The galaxy appears to be a relatively smooth, elliptical type. It exhibits a centrally concentrated luminosity profile with a gradual falloff towards the outer edges. The galaxy appears mostly featureless with no discernible spiral arms or dust lanes evident in this image. It possesses a high degree of roundness. There is no visible evidence of any major merger events or significant tidal disturbances, or any close companions. The color index suggests the stellar population is comprised of older stars. The galaxy's overall morphology points towards it being a relaxed system with a fairly quiescent star formation history.
