The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a largely elliptical morphology, deviating little from a circular shape. The core region is bright and appears to be a yellowish-orange hue, which may indicate an older stellar population. The outer regions of the galaxy fade gradually into the background sky, with a subtle transition from yellow-orange to a slightly more blueish tint as you move away from the center. No distinct spiral arm structures or prominent dust lanes are discernible in the image. There are hints of some minor asymmetry in the outer reaches of the galaxy, but it is not strongly indicative of a major ongoing merger event. The overall appearance suggests a galaxy that has largely exhausted its gas reservoir and is in the process of passively evolving.
