The galaxy presents as a single, fairly compact object with a smooth, elliptical morphology. The core exhibits a bright, concentrated luminosity, indicative of a substantial stellar population. There's a gradual decrease in light intensity from the center outward, forming a diffuse halo surrounding the core. Color gradients are subtle; the central region appears slightly yellow-white, transitioning to a bluish-white in the outer regions. The overall structure lacks any readily discernible spiral arms or distinct features like dust lanes. The smoothness and lack of significant disturbances suggest that the galaxy is likely a relaxed system, undisturbed by recent major mergers.
