The galaxy appears to be undergoing a significant merger event. There are at least two distinct nuclei visible, suggesting that two galaxies of substantial size are in the process of coalescing. The overall structure is highly disturbed, with tidal tails extending outwards, indicating strong gravitational interactions. The northernmost component appears more elliptical and exhibits a smoother morphology. The other component appears more irregular and potentially disc-like. There are a few blueish knots visible within the galaxy, suggesting areas of active star formation that may have been triggered by the interaction. The system appears to be relatively massive and luminous. Dust lanes are not easily discernible, but the irregular morphology suggests a potentially high dust content distributed throughout the system.
