The observed galaxy presents as a merging system characterized by significant tidal disruption. Two primary galactic nuclei are discernible, both exhibiting a yellowish-white coloration indicative of an older stellar population. Extended, diffuse tidal tails emanate from these nuclei, displaying a bluish tinge suggestive of more recent star formation. The overall morphology is highly irregular, lacking a well-defined disk structure. Intense gravitational interactions appear to be significantly distorting the galactic shapes. The system exhibits a substantial spatial extent. Evidence for on-going major merger activity is strong. 
