The galaxy presents a generally smooth morphology, with a concentrated central bulge. The galaxy appears elliptical in shape, although there may be a slight hint of a disk component. There is a relatively uniform distribution of light across the galaxy, with the brightest regions concentrated in the core. There is no evidence of strong spiral arms or significant dust lanes. The galaxy's color suggests a population dominated by older stars, with a possible lower rate of current star formation. The galaxy shows no evidence of tidal features, major disturbances, or ongoing mergers.
