The galaxy presents as a disturbed system. Two relatively bright, unresolved cores are apparent in the image, suggesting a possible ongoing or recent merger event. The overall shape appears amorphous with faint tidal features or extended diffuse light surrounding the central region. The color indices suggest the presence of an older stellar population within the core regions, while some bluer regions might indicate areas of recent star formation triggered by the interaction. The system exhibits a complex morphology indicative of strong gravitational interactions.
