The galaxy presents as a relatively smooth, elliptical-like structure. The light distribution appears centrally concentrated, with a gradual decrease in brightness moving outwards from the core. There is no immediately discernible disk-like structure or spiral arm morphology. The color profile is generally consistent across the galaxy, lacking distinct blue or red regions suggestive of differing stellar populations or recent star formation activity. The overall appearance suggests a lack of ongoing major interactions or mergers, with minimal visible disturbances to the galaxy's overall form. The galaxy is rather round in shape.