This galaxy exhibits a largely smooth morphology, appearing elliptical in shape with a high degree of central concentration. The core region emits strongly across observed wavelengths, with a distinct yellow hue. The light smoothly transitions outward and fades with a subtle red shift. No prominent spiral arm structures or significant dust lanes are discernible, suggesting an older stellar population and a relatively quiescent star formation history. There is a slight indication of minor asymmetry, but it could also be attributed to image artifacting. Overall, the galaxy presents as a well-defined, relatively undisturbed system.
