The galaxy presents as a merging system, exhibiting significant morphological disturbance. A primary component displays a disk-like structure with discernible spiral arms. These arms appear loosely wound. A central bulge is visible. A prominent bar feature crosses the central region of the primary galaxy. The secondary component exhibits a more amorphous shape, indicating a late stage merging event. Tidal tails are apparent. The overall color suggests ongoing star formation, particularly concentrated in the spiral arms of the primary component.