The galaxy appears to be a relatively smooth, elliptical galaxy, approximately 8.4 kpc in radius. It exhibits a primarily smooth morphology with a slight elongation. The central bulge is dominant and bright, with a yellow-red hue, indicating an older stellar population. There is a subtle, faint disk present and there is likely little ongoing star formation. Based on the slight disturbances to the light in the galaxy, it is probably not undergoing a major merger currently. There is a very small possibility that there is a minor disturbance happening. 
