The galaxy appears as a pair of interacting or merging systems. The larger component displays a smooth, centrally concentrated light profile, potentially indicative of an elliptical galaxy or a bulge-dominated spiral. The smaller component presents a more irregular shape, possibly a dwarf galaxy or a tidal feature resulting from the interaction. Overall, the system exhibits a yellowish-red hue, suggesting a population of older stars and/or significant dust obscuration. There's a hint of blueish color surrounding the galaxy.
