The object appears to be a galaxy undergoing a significant merger event. There are two primary concentrations of light, suggestive of galactic nuclei. The morphology of the overall system is highly irregular, exhibiting tidal features and disturbed structures, indicating strong gravitational interaction. A significant fraction of the light is concentrated in a more diffuse halo surrounding the central concentrations. There is a distinct tail-like extension emanating from one of the nuclei which suggests significant tidal forces at play. The overall color is primarily yellow-red, indicating an older stellar population, although bluer hues are visible in certain regions, possibly indicative of more recent star formation triggered by the merger. Based on the disruption observed, the merger is likely in a late stage.
