The galaxy presents as a system undergoing a significant merger event. Multiple galactic nuclei are observed, with three distinct luminous concentrations visible within the system. The morphology suggests a disruption of the original galactic structures, with a high likelihood of tidal features, though the resolution limits a definitive identification. The colors of the nuclei vary, implying differences in stellar populations or dust content within each component. The overall light distribution is relatively smooth, hinting at a potential transition towards a more relaxed, elliptical morphology in the distant future. Star formation is likely suppressed due to the ongoing interaction. 
