The galaxy presents a flattened, disk-like morphology when viewed from our observational perspective. The central region exhibits a relatively smooth and concentrated luminosity profile, appearing significantly brighter than the outer regions. The color distribution suggests differential stellar populations, with a slightly bluer hue in the central region, indicative of younger, hotter stars, and a tendency towards redder colors in the outer disk, indicating older, cooler stars. Hints of disturbances or tidal features are present, most obviously to the top and bottom of the galaxy. There are also slight disruptions to the symmetry of the main disk, indicating possible interactions or recent merging events. Overall, the galaxy appears to be a disk galaxy, which is relatively undisturbed but may be undergoing some form of interaction or merger.
