The galaxy presents as a relatively smooth, elliptical-like structure. A prominent central bulge exhibits a concentrated luminosity gradient, appearing yellowish-orange in color. The luminosity decreases radially outward from the core. There is little to no resolved spiral arm structure. The outer regions exhibit a more diffuse and less structured halo or envelope. The overall color profile suggests a population dominated by older stars, with indications of a low rate of current star formation. The morphology indicates a high probability that the galaxy has not experienced any recent major mergers, with a shape that is in between being round and in between elongated. Evident is a slight degree of disturbance, suggesting possible minor interactions.
