This galaxy appears to be undergoing a significant interaction or merger event. Its morphology is highly disturbed, with evidence of tidal features and asymmetric light distribution. Two distinct luminous regions are observed, possibly representing the merging nuclei of the progenitor galaxies. These regions exhibit different color profiles, with one appearing more reddish, indicating a potentially older stellar population or higher dust obscuration, and the other displaying bluer hues, possibly indicating younger stars. There are areas with diffuse, lower-surface brightness emission extending outward. Overall, the galaxy appears to be in a late stage of merging, with the disk structures highly disrupted. Low star formation.