The galaxy presents as a system undergoing a significant merger event. It is elongated in shape, with a central, brighter region exhibiting a yellowish-red hue suggestive of an older stellar population. This central region is moderately smooth and round, indicating a degree of dynamical relaxation, but substantial disturbances are present. Fainter components extend outwards from the central body, showing a bluer color suggesting ongoing star formation. The morphology is complex, with no clear spiral arm structures or well-defined disk. The overall appearance indicates a system with an estimated stellar mass around 10^10 solar masses, and a moderate rate of star formation.
