The galaxy presents as a generally smooth and rounded object. The light is concentrated toward the center, with a gradual decrease in intensity outward. The galaxy exhibits a reddish-orange hue, indicating a population of older stars. The galaxy has a smooth appearance, with no obvious spiral arms or bar structure visible. There is no visible evidence of active galactic nuclei activity or significant dust lanes. There are no apparent major merger features, tidal tails, or other signs of recent or ongoing interactions with other galaxies. Slight hints of bluer emission are seen in some regions, suggesting a small amount of recent star formation activity. The overall morphology is suggestive of an elliptical galaxy.
