The galaxy presents a complex morphology, characterized by significant disturbances. The central region appears relatively smooth, but a larger area appears to have a disk that may be disrupted. There are apparent tidal features, and a secondary nucleus-like structure that suggest an ongoing or recent merger event. The galaxy exhibits a mixed color profile. The central bulge appears to be a more intense red, and the outer disk shows a blue tint. The overall structure is irregular, indicative of gravitational interactions.
