The galaxy presents as a centrally concentrated object with a smooth, symmetrical morphology. Its light profile appears elliptical, with a gradual decrease in surface brightness moving outward from the core. The galaxy exhibits a yellowish hue, suggesting a dominant population of older stars with lower levels of ongoing star formation. No distinct spiral arms or features indicating recent major mergers are readily apparent. There may be minor distortions or some faint features, possibly small dust lanes or faint tidal features, but the overall structure is largely undisturbed. The object appears relatively compact, and the light is dominated by a redder core and a smoother, symmetric halo.
