The galaxy presents as a system undergoing a significant interaction or merger. A prominent feature is the presence of two distinct nuclei, suggesting two galaxies. The northern nucleus exhibits a distinctly yellow-orange hue, possibly indicating an older stellar population and/or significant dust obscuration. The southern nucleus is comparatively bluer and brighter, suggestive of a younger stellar population, possibly induced by the interaction with the northern galaxy.

The overall morphology is disturbed, lacking the defined spiral arms or elliptical structure. There appears to be a tidal tail or bridge of material extending between the two nuclei and beyond, further indicating an ongoing merger. A diffuse halo surrounds both galaxies, implying considerable disruption of the original galactic structures. The system appears to be relatively compact, with the majority of light concentrated within a small area.
