The galaxy in the image presents a clear, well-defined spiral structure. Multiple spiral arms extend outwards. The spiral arms appear loosely wound and lack a tight or distinct form, suggesting a later Hubble type. The presence of a bar structure is discernible across the central region of the galaxy, it appears to be strongly defined. 

The bulge component is small relative to the galactic disk. The disk is viewed at an oblique angle, it is not edge-on. The overall morphology is suggestive of a system currently experiencing a significant interaction. High likelihood of a merger event, showing signs of major disturbance.
