The galaxy presents a largely smooth, elliptical morphology. The central region exhibits a bright, concentrated core with a yellowish-white hue, suggesting a population of older stars. Moving outward from the core, the light gradually diffuses, forming an extended halo. There is only a slight hint of any features beyond this smooth profile, such as spiral arms or dust lanes. The overall color profile indicates that star formation is either minimal or not actively occurring at a high rate. The roundness of the galaxy indicates a low inclination relative to the observer's line of sight. There are no signs of any major mergers, but a minor disturbance cannot be ruled out.
