The galaxy presents as a relatively compact object. It exhibits a moderate degree of ellipticity, appearing somewhat elongated. A central bulge is discernible, characterized by a yellowish-white hue, suggesting a population of older stars. Fainter, bluer regions are observed extending outwards from the central bulge, likely indicating areas of more recent star formation. There appears to be a slight disturbance to the disk with some asymmetry present on one side suggesting a possible interaction or minor merger in the galaxy's history. The overall structure can be generally described as a disk galaxy, seen at a slight inclination.
