The galaxy appears to be undergoing a merging or interaction event. The primary galaxy displays an elongated morphology, suggesting it is either elliptical or a disk galaxy viewed at an angle. The light distribution is relatively smooth with a somewhat diffuse outer halo. There is evidence of a potential tidal tail or extended arm-like structure extending toward a secondary, smaller galaxy. The secondary galaxy appears more compact and circular. The overall color of the system is predominantly green, indicating significant star formation activity throughout. There are subtle indications of disturbances in the main body of the larger galaxy. The merger might be classified as minor, given the relatively small size differential between the two galaxies.
