The galaxy presents as a merging system, likely in the late stages of interaction. Two primary components are discernible: a larger, more diffuse component that appears relatively smooth, exhibiting a yellowish-white hue. The other component is slightly smaller and possesses a distinctly reddish-orange coloration. A faint, smaller object is noted below the merging system, and appears to be interacting as well. There appears to be significant tidal disturbance in the system, but an overall elliptical shape is still retained. The system is actively undergoing star formation, concentrated more heavily in what may be the nuclei. There are signs of an incomplete merger. 
