The galaxy appears to be a merging system, possibly undergoing a significant interaction. There is a discernible central region with a somewhat diffuse structure, suggestive of a disrupted morphology. Faint tidal features or streams emanate outwards from the central body, implying gravitational disturbance from a merger event. There is a degree of asymmetry present, suggesting that the system has not yet reached a state of equilibrium after the interaction. Color gradients are present within the galaxy, indicating differing stellar populations or dust distribution across its features. One of the merging galaxies appears to have an apparent disk-like structure, which has clearly been disrupted.
