The galaxy presents as a relatively smooth, somewhat rounded structure with a prominent central bulge. The core is a bright, concentrated region, suggesting a high density of stars. Moving outward, the intensity of light decreases gradually, forming a diffuse halo. There is a hint of a disk-like structure around the central bulge, evidenced by a slight flattening and elongation. The overall color appears yellowish-white, indicating a population of older stars. A faint bluish region is visible, which might indicate a more localized star forming region. There is no definitive evidence of spiral arms.
