The galaxy presents as an apparent merging system. Two distinct galactic nuclei are observed, one slightly larger and brighter than the other. These nuclei are connected by a faint bridge of diffuse material which seems to be being stretched between them. The system exhibits an overall elliptical morphology. The larger nucleus displays a yellowish hue, potentially indicating an older stellar population. A region of reddish emission appears between the two nuclei. This might be a region of intense star formation. Tidal distortions are subtle, suggesting the system is in the early to mid-stages of merging. 
