The galaxy presents as a relatively compact, elliptical morphology. Its light is concentrated towards the center, with a smooth, gradual decrease in brightness toward the outer regions. The core appears yellowish, potentially indicating an older stellar population. Faint blue-green hues are visible, suggesting a minor level of recent or ongoing star formation, though the overall star formation rate appears low. The galaxy is largely undisturbed, showing no evidence of major mergers or tidal disruptions. The shape is moderately round.
