The galaxy presents a morphology dominated by a smooth, spheroidal component, with a centrally concentrated bulge. There appears to be a notable disk-like structure that is experiencing some type of disturbance. The galaxy has a generally round appearance, though not perfectly spherical, leaning towards an intermediate ellipticity. There are traces of a possible minor disturbance, but they do not appear to dramatically disrupt the overall structure of the system. Indications of an interaction or potential merger with a secondary object appear possible within its immediate vicinity. The color of the galaxy is observed as primarily yellow, suggesting an older stellar population in the bulge. The estimated size suggests this galaxy to be moderately extended on the sky. Overall, this galaxy exhibits signs of moderate star formation rates.
