The galaxy presents as a relatively compact, elliptical-like system with a concentrated, bright core. A significant portion of the galaxy's light appears to be emitted from a central bulge, with a general smooth appearance in the primary body. There is an indication of an extended, fainter halo surrounding the central region. The observed color suggests a population dominated by older stars, with less evidence of recent or ongoing star formation. A slight asymmetry in the outer regions may suggest past or ongoing interactions with other galaxies.
