The galaxy appears to be a relatively smooth, elliptical or lenticular galaxy, exhibiting a predominantly yellow-orange hue suggesting an older stellar population and a lack of significant ongoing star formation throughout the majority of the galaxy. The morphology suggests it is a fairly rounded galaxy, with a possible slight elongation. There is a single bright spot, with a blue-green color, suggesting more recent star formation or an active galactic nucleus. There is no evidence of major mergers or significant disturbances in the overall structure; the galaxy appears relatively undisturbed.
