The galaxy presents as a well-defined elliptical morphology with a smooth, centrally concentrated light profile. The core exhibits a bright, compact emission region, suggesting a high stellar density. A gradual decrease in surface brightness extends outward from the core, forming a diffuse halo. The color gradient across the galaxy is subtle, transitioning from a slightly yellower hue in the central region to a redder color in the outer regions. No distinct spiral arms, dust lanes, or other prominent features are discernible in the image. The overall appearance is consistent with a relatively massive, evolved galaxy with ongoing, albeit potentially low-level, star formation.
