The galaxy presents a generally smooth, elliptical morphology. Its central bulge exhibits a bright, yellowish-white hue, suggesting an older stellar population. Fainter, bluer regions are observed extending outwards from the central bulge, indicating areas of more recent star formation. The galaxy is moderately elongated, but generally oval. There are no apparent strong tidal features or evidence of major mergers. Faint, diffuse light surrounds the central region of the galaxy, which could indicate an extended stellar halo. A small region with hints of spiral arms is visible, showing minor disturbances.
