The galaxy appears as a system undergoing a significant merger event. The morphology is highly disturbed, with evidence of multiple nuclei or bright clumps of stellar material. The overall shape is irregular, lacking a well-defined disk or spiral structure. The color profile suggests a mix of stellar populations, with some regions appearing redder, potentially indicative of older stars or dust obscuration. Tidal features, such as faint streams or extended halos, might be present, though the image resolution limits definitive identification. The system is relatively compact, with the interacting components in close proximity. Overall, the galaxy's characteristics align with those of a merging system in a relatively advanced stage of interaction.
