The galaxy appears to be in a late stage merger or tidal interaction with a companion galaxy. There is a significant disturbance of the primary galaxy's morphology. The system displays two distinct, luminous galactic nuclei, suggesting a dual-core structure. The light from the galaxy is primarily red and yellow, suggesting a relatively older stellar population with fewer young, hot stars. The morphology indicates a system that is not particularly disk-like, appearing smooth overall. The individual shapes of the galactic nuclei appear fairly round. The overall system is relatively compact.