The galaxy presents as a relatively smooth, elliptical-like structure, with a concentrated central bulge. The light distribution shows a radial decrease in intensity from the center outwards. There appears to be a hint of bluer light visible extending outward on the western side. This galaxy does not exhibit any strong signs of tidal disturbances or major ongoing mergers in this image, though a small feature is apparent extending off to the west. The galaxy is more rounded than it is elongated. The overall color suggests a population of older stars, though with hints of some ongoing star formation in the western extension.
