The galaxy appears to be a spiral galaxy undergoing a significant merger event. Distinct spiral arms are visible, although their structure is distorted, indicating gravitational interaction. The overall color is blue-white, suggesting recent or ongoing star formation. A moderate bulge is present at the center of the main galaxy. The interacting component is close, and of similar size to the primary component. Tidal tails or bridges are present between the interacting galaxies. The morphology indicates an active, possibly late-stage merger.
