The galaxy presents a somewhat disturbed morphology. The central region exhibits a concentrated, relatively smooth, yellowish-orange hue. Extending to one side of the center is a blue-tinted, diffuse feature, possibly indicative of tidal debris or a disrupted spiral arm. This blue region suggests the presence of younger, hotter stars due to ongoing or recent star formation. The overall shape appears to be an intermediate form between elliptical and disk-like, with notable disturbances suggesting either a recent or ongoing merger event. Evidence of faint, extended material surrounding the primary body hints at a complex interaction history.
