The galaxy presents a primarily smooth, elliptical morphology. There is a bright, centralized bulge region that dominates the overall light profile. A subtle, but noticeable color gradient can be seen, where the central region shows a yellow-white hue, indicating an older stellar population. There may be minor disturbances visible suggesting that the galaxy is potentially undergoing some kind of interaction or merger. Faint blue tinges are visible across the galaxy suggesting the presence of younger stars. It appears to be relatively compact with no clear spiral arm structure. The apparent round shape indicates that we may be observing the galaxy close to face-on.
