The galaxy exhibits an elliptical morphology, appearing largely featureless and smooth. The light distribution is centrally concentrated with a gradual decrease in intensity towards the outer regions, implying a relatively old stellar population. The galaxy displays a slightly elongated shape with an ellipticity of approximately 0.4, appearing somewhat flattened. The color profile suggests a redder core region, possibly indicative of a higher concentration of older stars and dust. The outer regions appear bluer, possibly reflecting a younger population of stars. There is no obvious presence of a prominent disk or spiral arm structure. The overall appearance is consistent with a relatively massive, evolved galaxy with minimal ongoing star formation.
