The galaxy presents as a system undergoing a significant merger event. Two primary galactic nuclei are visible, one exhibiting a bluer spectral profile and the other displaying a more yellow-red hue. This color differential suggests varying stellar populations and potentially differing levels of dust obscuration. A disturbed morphology is evident, with tidal features and irregular light distribution indicative of strong gravitational interactions. The overall shape is distorted, deviating significantly from a regular elliptical or spiral structure. The smooth fraction is significant but the presence of features suggests ongoing processes.
