The galaxy presents a primarily smooth morphology with a central bulge that is elongated, suggesting a possible elliptical or lenticular classification. The core region exhibits a bright, concentrated luminosity. The galaxy's light profile appears somewhat flattened, displaying a cigar-like shape. There is a slight suggestion of a disk-like structure but it is difficult to confirm due to the viewing angle and the dominant smooth texture. There may be some minor disturbances present in the outer regions, but overall there's no sign of a major ongoing merger or intense interaction. The galaxy color index suggests it contains relatively old stellar populations, with a low star formation rate. The overall structure indicates a relatively evolved system that has likely undergone significant processing of its gas content.
