The galaxy presents as an elliptical or lenticular structure with a centrally concentrated luminosity profile. The core region displays a smooth, yellowish hue indicative of an older stellar population. There's a subtle transition to a slightly bluer color in the surrounding area, implying the presence of younger stars, possibly within a faint, extended disk. Overall, the galaxy shows no signs of ongoing major mergers or significant tidal disturbances. It appears relatively undisturbed and relaxed in its morphology.
