The galaxy exhibits a complex morphology, appearing to be undergoing some form of interaction or disturbance. The central region is characterized by a relatively smooth, somewhat amorphous distribution of light, possibly indicative of a bulge component. A tidal feature emanates from this central region and is characterized by bright knot or clumps. This structure is elongated. These features suggest ongoing or recent merger activity, or at least a gravitational interaction with a smaller companion galaxy.

The overall color gradient indicates a mixed stellar population. The central area has a redder hue and the outer regions are bluer. This may suggest ongoing or recent star formation in these outer areas.
