The galaxy presents a generally disk-like morphology, although it exhibits features suggesting ongoing or recent interactions. The central region appears bright and relatively smooth, indicative of a prominent bulge or nucleus. A fainter disk extends outwards from the center.

The disk shows some asymmetry and disrupted features, with a hint of spiral arm structure on one side. These features could be the result of tidal interactions, such as a minor merger event. The color of the galaxy is slightly bluer in the disk and spiral arm regions and redder in the central bulge region, suggesting ongoing star formation within the disk. Overall, it appears to be a galaxy with a disturbed morphology, likely influenced by gravitational interactions.
