The galaxy presents an apparent morphology indicative of a system undergoing a merging event or significant interaction. The overall structure is complex and asymmetrical, lacking a clearly defined nucleus. It appears to consist of several distinct luminous clumps or nodes, suggesting multiple galactic cores or areas of enhanced star formation activity triggered by the interaction. Color gradients are observed, with some regions exhibiting bluer hues and others exhibiting redder hues, likely indicative of varying stellar populations and star formation rates within the system. The galaxy appears relatively smooth, with only subtle signs of tidal tails or strong gravitational distortions, though further investigation might reveal subtle signatures of past interactions.
