This galaxy exhibits a disk-like morphology, viewed at a noticeable inclination. The central region appears bright and concentrated, indicative of a significant stellar population and possibly an active galactic nucleus. Surrounding the central region is a less luminous, extended disk. The color gradient suggests variations in stellar populations across the galaxy, with bluer regions potentially indicating areas of active star formation. There is no obvious spiral arm structure and there may be a minor disturbance within the galaxy. Overall the galaxy is rather smooth.