The object appears to be a galaxy undergoing a major merger, or is a close interacting pair. The morphology suggests advanced stages of interaction. Two distinct nuclei are visible, characterized by concentrated, relatively red emission. Around each is a diffuse halo of greenish light, perhaps gas or intense star formation surrounding the cores, potentially triggered by tidal interactions. The overall structure is complex and disturbed, lacking a clear spiral or elliptical form. The integrated light from the galaxy is dominated by emission in the green and red parts of the spectrum. Tidal features appear to emanate from the main body, adding to the overall disturbed appearance.
