The galaxy presents as a spiral, exhibiting a flattened disk structure. Prominent spiral arms are observed extending from a central bulge region. The arms appear somewhat tightly wound. A bar-like structure appears to transect the central bulge. The bulge appears to be of moderate size, but is still relatively visible. There is no sign of active merging or tidal features, and the spiral structure appears relatively unperturbed, although some minor disturbance is possible. The color distribution suggests active star formation within the spiral arms. The galaxy's orientation is nearly face-on, allowing for detailed observation of its spiral structure. The disk exhibits a noticeable inclination from a perfect face-on view.
