The galaxy presents as a system undergoing a significant merger event. There appear to be two distinct nuclei. One nucleus presents a more yellow appearance than the other, while the other has a slightly whiter appearance. The overall shape is irregular, lacking a well-defined disk or spiral structure. Tidal features are visible, indicating gravitational interaction. These features extend outwards from the main body. Overall, the system exhibits a moderate degree of star formation, evidenced by the redder regions. The galaxy exhibits intermediate roundness. The observed morphology suggests a late-stage merger in progress.