This galaxy exhibits a complex morphology, appearing to be undergoing a significant interaction or merger event. The central region is characterized by a bright, somewhat amorphous core, possibly indicating a concentration of stellar populations and active galactic nuclei activity. There is a suggestion of disturbed disk features, implying tidal disruption from a secondary component. There are luminous clumps within the galactic body, these could be intense areas of star formation or dense regions of gas and dust. A faint halo surrounds the core, which suggests tidal tails of debris stemming from the interaction event. The overall colour profile indicates a variety of stellar ages, the central region is distinctly blue. The size of the galaxy, while difficult to precisely determine from this image alone, appears compact. The presence of a strong interaction signature suggests a dynamic system, potentially leading to a significant change in its overall structure and stellar populations over time. 
