This galaxy exhibits a distinct spiral structure, though the arms are not sharply defined. They appear somewhat diffuse. The galaxy presents a clear disk-like component.

There is evidence of an interaction or merging event. The primary body of the galaxy appears significantly distorted. There may be a secondary core or object involved in the interaction, suggesting it may be a merger in progress. The merging object could be of approximately equal brightness to the galaxy.

A bulge component is present, although it does not appear to be the dominant feature. The galaxy displays a yellow-orange hue overall.
