The object appears to be a galaxy undergoing a significant merger. Multiple distinct nuclei are visible, with disturbed and elongated tidal features extending outwards, indicating a gravitational interaction between two or more galaxies. There is a central concentration of light and material, with the overall structure showing an irregular shape as opposed to a clear disk or elliptical form. Patches of bluer light are present, which may indicate ongoing star formation activity within the system. The redder colors present likely indicate a older stellar population with lower levels of active star formation.
