This galaxy presents as a moderately luminous system with a fairly smooth overall morphology. The light profile suggests a concentration of older stars toward the central region, displaying a yellowish-orange hue, which likely indicates an older stellar population. The galaxy has a somewhat elongated shape, appearing elliptical but not extremely so. Fainter, bluer light extends outward from the core region, indicating the presence of a younger stellar population and possible star formation, though not at a significant rate. There are no obvious signs of major disturbances or ongoing mergers. The overall structure appears relatively relaxed and settled, which indicates that it is not experiencing major interaction with other galaxies. 
