The galaxy presents as a slightly elongated, primarily smooth, elliptical morphology. There appears to be a subtle, disk-like structure, though it does not dominate the overall appearance. The galaxy's color profile suggests a redder hue, indicating a population of older stars and a relatively lower rate of ongoing star formation. The light distribution is centrally concentrated, with a gradual decrease in luminosity towards the outer regions. There is no apparent major disturbance or ongoing merger activity, although a slight asymmetry is observed, which may be a sign of a past minor interaction. Overall, the galaxy appears to be a relatively massive, evolved system with little current star formation.
