The object presents as a spiral galaxy undergoing a significant merger event. Two distinct galactic nuclei are visible, one more obscured than the other, suggesting differential dust obscuration or varying stellar populations. The spiral arms emanating from both nuclei are highly distorted, exhibiting a flocculent morphology. The arm structure is complex and asymmetric, with evidence of tidal tails extending from the main galactic body. A considerable amount of star formation appears to be occurring within these tails and arms, indicated by the patchy distribution of bluish regions. Redder regions may indicate either dust obscuration of star-forming regions or an older stellar population. There is evidence of a bar-like feature within at least one of the merging galaxies. The system is highly disturbed, indicating an advanced stage in the merging process.
