The galaxy exhibits an irregular morphology, suggestive of an ongoing or recent interaction or merger event. There appear to be two distinct nuclei, both displaying a yellowish hue. Faint tidal features or distortions are present, extending outwards from the main body, which supports the merging hypothesis. The overall color of the galaxy appears somewhat red, potentially indicating an older stellar population or significant dust obscuration. The system appears to be undergoing significant disturbance.
