The galaxy exhibits a morphology suggestive of an ongoing merger. Two distinct luminous regions are apparent. One region presents a relatively smooth, round appearance with a bright, concentrated core, indicating a possible spheroidal component. The second luminous region displays a more elongated, irregular structure, potentially indicating a disk-like component or tidal tail. The overall color of the system indicates a mix of stellar populations, with some regions appearing bluer, possibly indicative of younger stars or active star formation, while others appear redder, suggesting older stellar populations. The relative proximity of these two regions, along with their distorted shapes, suggests a strong gravitational interaction and a system in the late stages of merging.
