This galaxy exhibits characteristics suggestive of a system undergoing a significant merger. The morphology displays multiple nuclei or centers of concentrated light, indicating a disruption of the original galactic structure. A considerable fraction of the galaxy appears smooth with a lack of well-defined spiral arms or a prominent disk, though the presence of certain disturbed disk features are still present. The overall shape is somewhat rounded, but a distinct tidal tail or plume extends from the main body, composed of diffuse material, likely stars and gas, pulled away by gravitational interactions. The light from the object appears fairly uniform.

A region of intense blue activity is also visible. This is likely due to ongoing or recent bursts of star formation.
