The galaxy presents as a multi-component system, likely undergoing or having recently undergone a merger. Two primary luminous concentrations are observed, suggesting either two distinct galactic nuclei or a single nucleus with significant off-center star formation. One concentration exhibits a bluer color profile, while the other is noticeably redder, indicative of differing stellar populations or dust obscuration. A faint, diffuse halo of light surrounds the central components, possibly tidal debris or a common envelope from the interaction. Morphologically, the system does not exhibit a clear disk structure, but a perturbed, irregular shape. There is evidence of disruption, with streams or tails of material extending from the main body. Based on its apparent color and morphology, the galaxy appears to be a relatively massive system.
