The galaxy presents as a relatively smooth, elliptical-like structure. The color profile appears yellowish-white, suggesting an older stellar population. There is a slight elongation visible, with the galaxy’s shape deviating somewhat from perfectly circular; appearing more "in between" in its roundness. No prominent spiral arms or significant dust lanes are discernible in the image. The galaxy's morphology does not indicate any current major merger activity, though a minor disturbance is possible. Overall, the galaxy exhibits characteristics of a quiescent, relatively evolved system.