The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a largely elliptical morphology with a high degree of rotational symmetry, and it looks to be somewhere in between round and elliptical. There is little visible evidence of spiral arm structure or significant dust lanes. A color gradient is observed, with the central region appearing yellower, suggestive of an older stellar population. The outer regions are comparatively redder. There is a hint of some minor disturbance in its shape but it is overall not exhibiting signs of a major ongoing merger. The overall light profile indicates a high likelihood of an older galaxy, and there are no indicators of significant star formation from the image.
