The galaxy presents as a flattened, disk-like structure with a prominent, bright central bulge. It is observed at a slight inclination, providing a partial view of its overall morphology. The light distribution appears relatively smooth, with a higher concentration of luminosity in the central region and a gradual decrease in brightness towards the outer edges. The color gradient suggests a stellar population that is more evolved in the bulge, indicated by the yellowish hue, and a bluer hue at the rim which might suggest the presence of a younger stellar population and/or ongoing star formation activity. The overall structure is largely undisturbed, showing no prominent tidal features, distortions, or signs of major merger activity. Subtle asymmetries might be present, which are potentially indicative of minor interactions or internal dynamic processes.
