The galaxy presents a largely smooth, elliptical morphology. It appears nearly circular in projection. The central region exhibits a high degree of luminosity, suggesting a dense concentration of stars or an active galactic nucleus. Proceeding outward from the core, the luminosity decreases gradually. The colour gradient transitions from a yellowish-white core to a redder halo. There is no discernible spiral arm structure, or prominent dust lanes visible. Subtle irregular features may indicate potential past or ongoing minor interactions. The galaxy overall appears relatively undisturbed, suggesting it is not currently undergoing a major merger event.
