The galaxy presents an elliptical morphology, exhibiting a smooth and centrally concentrated light profile. The core appears bright and nearly spherical, gradually fading into a more diffuse halo. The galaxy's color suggests a population of older stars, dominated by redder wavelengths. No distinct spiral arms or significant dust lanes are readily apparent within this imaging. There is a lack of prominent star-forming regions. The galaxy appears relatively undisturbed, with no signs of major mergers or tidal disruptions. It displays a roughly round shape, with only a slight deviation toward an elongated form.