The galaxy presents as a relatively smooth, centrally concentrated object, with a largely elliptical morphology. There is a bright, yellowish core, suggesting a significant population of older stars within the central bulge. The outer regions of the galaxy exhibit a gradual decrease in surface brightness, transitioning into a diffuse halo. Although the overall appearance is smooth, there may be some minor disturbances visible in the outer regions, indicating potential interactions with smaller objects, although these are not clear. Color gradients are subtle, but suggest a bluer stellar population at the edges of the central bulge. No clear spiral arm structures are apparent, reinforcing the classification of this galaxy as a relatively early-type system. Overall, the galaxy is classified as smooth.
