The galaxy presents as a disk-shaped structure with a smooth, centralized bulge. The color profile suggests a relatively old stellar population dominating the bulge, exhibiting a yellow-orange hue, while bluer tones are weakly observable at the very edge of the galactic disk. The smooth light distribution implies a lack of active star formation within the bulge, which is consistent with an elliptical galaxy. Overall, the galaxy appears to be in a relatively undisturbed state, with no apparent tidal features or major distortions in its morphology. The observed inclination provides a view of the disk structure but obscures a clear determination of spiral arm presence.
