This galaxy exhibits a prominent disk structure, and the presence of spiral arms is strongly suggested. The arms appear to be tightly wound in many locations. There appears to be two main components, one of which is a disrupted spiral galaxy in the process of merging. The bulge size of the larger component appears moderate in size and is dominant, however the presence of a tidal tail suggests that they are interacting. There is a possible bar structure visible in the larger component, its prominence seems of medium strength. Indications of tidal disruption are seen, which suggests an on-going or recent merger event.
