The galaxy exhibits a complex morphology, suggestive of an ongoing or recent interaction. The primary component appears relatively smooth and diffuse, potentially indicating an elliptical galaxy. However, there is a clear secondary component that is more compact and possesses a bluer color, implying a region of active star formation. A tidal tail or bridge-like structure seems to connect these two components, hinting at a gravitational interaction. The overall shape deviates significantly from a simple elliptical or spiral form; there is a clear disturbance within the structure. The galaxy is relatively faint in the redder bands compared to the bluer bands, suggesting a moderate redshift. The system appears to be undergoing some type of merger event.
