The galaxy appears as a somewhat diffuse, elliptical object. Its core region exhibits a concentrated luminosity profile, indicating a possible central bulge. The overall color suggests a relatively evolved stellar population, with a bias toward redder wavelengths. There is a subtle hint of disk-like structure, though it's not clearly defined, the morphology is primarily smooth. The object shows no obvious signs of tidal features or major disturbances, suggesting it is not currently undergoing a major merger event, though minor disturbances cannot be ruled out. The relative smoothness supports the conclusion that it is an early-type galaxy.
