The galaxy presents as a relatively smooth, centrally concentrated object, displaying an elliptical morphology. The light profile indicates a spheroid-dominated structure with a gradual decrease in surface brightness from the core outwards. The core exhibits a yellowish hue, possibly indicating an older stellar population. There is no prominent disk structure visible. No spiral arms or significant dust lanes are discernible. There appears to be a lack of irregular features, suggesting that the galaxy is relatively undisturbed and possibly quiescent in terms of star formation.
