The galaxy presents a complex morphology, appearing to be undergoing a significant interaction or merger event. A primary, relatively smooth component, exhibits a blueish tint, suggestive of active star formation. Adjacent to it, a more yellowish-orange component is visible, potentially indicating an older stellar population. This orange component is also quite smooth, suggesting that this could be an elliptical galaxy or the bulge of a spiral galaxy. A fainter, reddish region is visible near the orange galaxy and may be a region of extremely active star formation, possibly triggered by the interaction. The overall structure suggests a system disturbed from equilibrium, likely due to gravitational interactions. These interactions could be leading to elevated star formation rates within the system, particularly in the bluer, primary component, and causing a distorted or elongated shape in the overall galactic structure.
