This galaxy appears to be undergoing a significant interaction. There are two distinct luminous regions visible, both exhibiting a slightly elongated morphology. The larger region presents a smoother appearance, with a yellow-orange hue suggesting an older stellar population. In close proximity, the second region shows a more irregular shape and a bluer, more diffuse glow indicative of recent or ongoing star formation. The overall structure displays possible tidal features or distortions, hinting at a recent or ongoing merger.
