The galaxy presents a smooth, elliptical morphology. The light distribution is highly concentrated and centrally bright. There is a suggestion of ongoing or recent merger activity. The galaxy appears slightly disturbed, potentially indicating an interaction with another galactic object. The main body exhibits a rounded shape, with the possibility of a minor tidal tail or irregular feature. There is minimal visible structure such as spiral arms or a well-defined disk. The color index suggests a population dominated by older stars, with some presence of younger, star-forming regions.
