The galaxy presents as a largely smooth, centrally concentrated object. Its color profile suggests it is comprised of older stellar populations, with a yellowish-red hue dominating. There is a slight color gradient, transitioning from a brighter, more yellow-white core to a more reddish outer halo. No distinct spiral arm features or pronounced dust lanes are visible. Overall, the galaxy appears relatively undisturbed, showing no obvious signs of a major merger event or significant tidal interactions.
