The galaxy presents as a system undergoing a significant interaction or merger. The primary body exhibits a centrally concentrated bulge, though its morphology is somewhat irregular. A prominent tidal tail extends outward, exhibiting bluer colors indicative of on-going star formation. The disk component appears disrupted, possibly due to gravitational interactions. The color gradient suggests a distribution of stellar populations, with the central bulge potentially dominated by older, redder stars, and the outer regions showing evidence of younger, bluer stars. Overall, the galaxy displays signs of a dynamic and evolving system.
