This galaxy appears to be undergoing a significant interaction, possibly a merger. The morphology is disturbed, with an elongated structure indicating tidal forces are at play. There appear to be at least two distinct, bright nuclei or concentrated regions of star formation within the system, suggesting either a recent or ongoing merger event between two galaxies. The color gradient indicates active star formation, particularly within the concentrated regions of the galaxy. There is a notable tail-like structure extending from the main body, suggestive of material stripped away during the interaction. While there is significant disturbance, hints of a spiral structure are present, likely a residual structure being distorted by this gravitational interaction. Overall, this is a complex system in a dynamically active phase.
