The galaxy exhibits a complex morphology, appearing as a system undergoing a possible interaction or merger event. The primary component presents a somewhat elliptical profile, though its structure shows signs of significant disturbance. There is an irregular shape with a possible tidal tail or bridge emanating from the main body. The color suggests a evolved stellar population, and the size seems relatively large, with an estimated effective radius on the order of tens of thousands of light years. The system appears to be actively forming stars, albeit at a relatively low rate.
