The galaxy appears to be undergoing a significant interaction or disturbance, possibly a merger. The overall structure is irregular and asymmetric, lacking a well-defined nucleus or spiral arm structure. There are indications of tidal features or extended diffuse emission extending from the main body of the galaxy. The light distribution is uneven, with patchy regions of higher intensity embedded within a more diffuse, lower surface brightness background. The color gradients suggest variations in stellar populations, with some regions appearing bluer indicating recent star formation, and other regions appearing redder indicating older stellar populations or dust extinction.
