The galaxy presents a largely smooth, elliptical morphology. The central region exhibits a concentrated, bright yellowish hue, indicative of an older stellar population. There is a subtle radial decrease in brightness from the core outwards, transitioning into a fainter, more diffuse halo. No distinct spiral arms or bar structures are discernible. The overall structure appears undisturbed, lacking signs of major mergers or tidal interactions. The galaxy's round shape dominates its overall appearance, suggesting a high degree of sphericity.
