The object presents as a disturbed system, likely a galaxy merger in progress. Two distinct, bright nuclei are visible, suggesting that the progenitor galaxies have not fully coalesced. The overall morphology is irregular and lacks clear spiral arm structure. There's a slight colour gradient between the nuclei suggesting differing star populations or dust content. Faint, diffuse light surrounds the bright cores, indicating a stellar halo likely formed from tidal stripping during the interaction. A noticeable asymmetry exists, possibly due to unequal mass ratios of the original galaxies.