This galaxy appears to be an elliptical, smooth galaxy with little to no spiral arm structure. The galaxy is centrally concentrated, with a high degree of circular symmetry. The overall color profile suggests a population of older stars, exhibiting a reddish-orange hue with a bright center. There may be some evidence of minor disturbances, such as a slight irregularity in its morphology, but appears to be isolated and not currently undergoing major mergers.