The galaxy presents as an elliptical morphology, although some disk-like features may be present. The core is bright and concentrated. The galaxy exhibits a noticeable tilt relative to our line of sight, which may give insight into its 3D shape, although with more information, it may be considered to be closer to face-on. There is a distinct color gradient, with the central bulge appearing more yellow/white, and the outer regions exhibiting bluer tones. This suggests ongoing star formation. Faint extensions may exist, indicating possible tidal interactions or recent mergers. The overall light distribution is smooth and diffuse, with no prominent spiral arms visible.
