The galaxy presents an irregular morphology, suggestive of a system undergoing or having recently undergone a merger event. Two distinct luminosity concentrations are observed. The brighter and more compact concentration appears to be largely spheroid in shape, with a yellow to green hue. The other concentration is more amorphous, with lower surface brightness, and displays a bluer color profile. There is evidence of tidal features, indicating possible disruption of the main galactic structure. These observations indicate potential ongoing star formation within both components of the interacting system. The overall light distribution is complex, lacking a clear central bulge or disk component, further supporting the hypothesis of a dynamically disturbed system.
