This galaxy presents as a generally smooth and elliptical structure. It exhibits a bright, concentrated central bulge, suggestive of an older stellar population and a potential supermassive black hole. The overall color is slightly reddish, likely due to the presence of older, cooler stars dominating the light output and some dust obscuration. There's a faint, diffuse halo surrounding the central region, which implies an extended distribution of stars and possibly globular clusters. There's a subtle hint of a disk-like structure, but the dominant morphology is that of an elliptical galaxy, likely undergoing only minor interactions.
