The galaxy appears to be undergoing a merger. Two distinct, roughly elliptical components are visible. One component displays a warmer, reddish-orange hue, suggesting an older stellar population or significant dust obscuration. The other component exhibits a slightly bluer color, potentially indicative of ongoing star formation or a younger stellar population. The morphology is disturbed, with some tidal features possibly present, though the image resolution limits detailed analysis. Based on the overall red color of the system, there appears to be a significant amount of older stars, or obscuring dust, suggesting that the merging components are relatively massive.
