The galaxy presents as a somewhat elliptical morphology with a bright, concentrated central bulge exhibiting a yellowish-white hue. The surrounding disk appears less structured, presenting a smoother distribution of light. The light from the disk is slightly bluer than the central bulge, suggesting ongoing star formation. A faint, diffuse halo is present around the main body of the galaxy. There are some disturbances that may suggest a previous merger. Overall, the galaxy is more smooth and has fewer features that are identifiable.
