The galaxy presents as a relatively smooth, elliptical or lenticular structure, with no prominent spiral arms or distinct features. Its overall shape appears elongated, with a noticeable bulge that exhibits a strong concentration of light. The light profile seems to follow a Sersic profile, with the index suggesting a somewhat intermediate shape between a pure exponential disk and a de Vaucouleurs profile. The color is generally yellowish, hinting at a population of older stars. The axial ratio indicates a flattened shape, though it is unclear if this is an intrinsic property or due to projection effects. There is no obvious sign of recent merging activity or tidal disturbances based on morphology. The galaxy's effective radius is relatively compact. Based on the relatively smooth appearance, the galaxy is likely in a late stage of its evolution.
