The galaxy presents a largely smooth, elliptical morphology. The central region exhibits a concentrated luminosity, appearing a yellowish-white hue. The color suggests a population of older stars dominating the core. Moving outward from the core, the color subtly shifts towards redder tones, indicating a continued presence of older stellar populations. There's no discernible spiral structure or prominent disk. Overall, the galaxy appears relatively undisturbed with no signs of recent major mergers or tidal disruptions and appears to be in a relatively quiescent state regarding star formation.
