The galaxy presents a largely smooth, elliptical morphology. It exhibits a concentrated central bulge, transitioning into a diffuse halo. The color profile is characterized by a redder hue within the central regions, suggestive of an older stellar population, while the outer regions show a slight shift toward bluer tones. There are no readily apparent spiral arm structures or dust lanes. The overall appearance is consistent with an evolved system. The galaxy appears isolated, showing no evidence of a major merger. There is a slight chance it could be experiencing a minor disturbance, but is more likely just a smooth elliptical galaxy.
