The galaxy presents as a system undergoing a major merger or experiencing significant tidal interactions. Two distinct nuclei are visible, each possessing a concentrated central bulge exhibiting a yellowish-orange hue. Diffuse, bluer material surrounds these central regions, suggesting ongoing star formation. The overall shape is irregular, with an elongated structure indicative of gravitational disturbance. There is a faint, tidal bridge or stream of material connecting the two main galactic components and surrounding them, reinforcing the interpretation of a merging system with significant tidal forces at play. The galaxy presents no clear spiral arm structure; the system is highly disrupted.
