The galaxy presents a generally smooth, elliptical morphology. The light distribution is centrally concentrated, with a gradual decrease in surface brightness outwards. The color index suggests a population dominated by older stars, giving it a yellowish-red hue. There is no apparent evidence of spiral arm structure, distinct dust lanes, or significant star-forming regions. The galaxy is moderately bright, suggesting a substantial stellar mass. Its shape is slightly elongated. Based on the overall characteristics, it appears to be a relatively evolved system with minimal ongoing star formation.
