The galaxy presents as a merging system, exhibiting signs of gravitational interaction. It's comprised of what appear to be three distinct luminous regions. Two larger, more diffuse regions are positioned closely together, suggestive of a major merger in progress. These regions display a somewhat smooth morphology, with possible tidal features or distortions evident, although low resolution obscures detailed analysis. A smaller, more compact region is situated some distance away, possibly another galaxy involved in the interaction or a tidal dwarf galaxy forming from the debris of the collision. The overall color appears relatively red, indicating an older stellar population and potentially suppressed star formation within the main bodies of the merging galaxies. The system appears to be undergoing a significant dynamic event, dramatically altering the structure and potentially influencing the future evolution of these galaxies.
