The galaxy presents a predominantly smooth, elliptical morphology. Its core exhibits a concentrated, bright profile, indicative of a substantial stellar population density. Moving outward from the core, the light profile diffuses gradually, suggesting a decreasing stellar density with increasing radius. There is minimal discernible substructure, such as spiral arms or prominent dust lanes. A slight color gradient is apparent, with the core exhibiting a yellower hue compared to the outer regions, which appear more greenish in the color channels used. This may indicate a higher concentration of older stellar populations in the nucleus. The galaxy’s shape deviates slightly from perfect circularity, displaying a minor elongation. There is no apparent interaction with any other galaxy. Overall, this appears to be a fairly undisturbed elliptical galaxy.
