The galaxy appears to be an elliptical galaxy with a relatively smooth light distribution and a somewhat circular morphology. There are no distinct spiral arms or obvious dust lanes. There appears to be a bright central bulge or nucleus, and the color gradient suggests a population of older stars dominates, particularly in the central region. Some blue light is distributed throughout the galaxy, particularly in the outer edges, suggesting some ongoing star formation, albeit at a relatively low rate. There is no evidence of any major mergers or significant tidal disturbances.
