The galaxy appears to be undergoing a significant merger event, likely past the initial contact phase. Two distinct galactic nuclei are visible, both displaying a relatively smooth, concentrated morphology, however both are greatly distorted. The nuclei are separated by an area of diffuse light, suggesting tidal interactions and stellar stripping between the two galaxies. A significant portion of the galaxy exhibits a disturbed morphology, with prominent tidal tails extending outward, indicative of strong gravitational interactions. These tails appear diffuse and spread out. Some bluer tinges may be visible, which indicate a small amount of star formation may be occurring. The overall shape of the merging system is irregular, far from an elliptical form. 
