The galaxy displays a complex morphology, suggestive of an ongoing or recent interaction. A bright, centrally concentrated region, approximately circular in shape, exhibits a yellowish-green hue, potentially indicating an older stellar population. Emanating from this central region are fainter, bluish extensions or features, hinting at possible spiral arm structure or tidal debris. One of the extensions appears to be a distinct tidal tail, and another brighter region to the top right of the main body of the galaxy. The galaxy does not appear perfectly symmetrical, its morphology is noticeably disturbed. The overall visual impression is of a system undergoing a gravitational perturbation or merger event.
