The galaxy exhibits a complex morphology, appearing as a merging system or a galaxy with significant tidal disturbances. A dominant, relatively smooth, central component is observed, with a yellowish-white hue, suggesting an older stellar population. Adjacent to this central structure, a more diffuse, elongated feature extends. This feature displays a reddish-orange color gradient, hinting at ongoing star formation or dust obscuration. Overall, the galaxy appears to be in a dynamic state.
