The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a bright central bulge which diminishes in luminosity gradually towards its outer edges. The morphology appears largely undisturbed, with no apparent major mergers or tidal features. The object is elongated with a ratio of approximately 2:1, though it is not cigar-shaped. Overall, it is an evolved galaxy, likely with low ongoing star formation activity. The galaxy appears to be a significant mass, based on its absolute magnitude and the extent of the luminous matter.
