The galaxy appears to be undergoing a significant interaction or merger event. A central, relatively smooth component exhibits a yellowish hue. Extending outward, a more diffuse, bluish structure is observed, which is indicative of ongoing or recent star formation. This bluish region is irregularly shaped, suggestive of tidal features resulting from gravitational interaction. The central region presents a moderate degree of roundness and does not appear highly elongated. The overall morphology indicates a system that is not relaxed and is in a state of dynamical disturbance.
