The galaxy presents as a generally smooth, elliptical morphology. Its color profile is predominantly yellowish-orange, indicating a significant population of older stars and a relatively low rate of current star formation. The light is concentrated towards the center of the galaxy, suggesting a dense nucleus. The outer regions appear fainter, with a gradual decrease in luminosity as one moves away from the core. There is a subtle disk structure visible, with the galaxy appearing somewhat flattened along one axis. There is no obvious evidence of spiral arms or significant dust lanes. The overall impression is of a mature galaxy with a well-established structure, showing no signs of a major merger event, though there may be subtle disturbances in the outer regions.
