The galaxy appears to be a lenticular or early-type spiral galaxy, viewed at a high inclination angle. It presents a smooth, elliptical light distribution with a noticeable bulge. There is a disk structure present but it is nearly edge-on. The central region of the galaxy exhibits a brighter, more concentrated luminosity profile than its outer regions, showing a significant bulge. There is some asymmetry visible in the galactic disk. Color gradients are observed, with the core appearing yellower and the outer regions exhibiting a bluer hue, potentially indicating variations in stellar populations or dust content. The overall structure suggests a relatively evolved system with ongoing but subdued star formation.
