The galaxy presents as a smooth, elliptical-like structure. The central region exhibits a bright, concentrated luminosity with a yellow-orange hue, suggesting an older stellar population. The overall shape approximates an ellipse, elongated along one axis. The edges appear to fade gradually into the background, with no distinct features of spiral arms or prominent dust lanes discernible. There are no major disturbances or merger signatures visible, implying a relatively undisturbed morphological state. A subtle blue-ish color gradient can be seen on the outer regions, possibly indicating younger stars, but this may also be a point spread function artifact from the central emission.
