The galaxy presents as a centrally concentrated object with a smooth, elliptical morphology. The core region exhibits a bright, yellowish-white luminosity, suggesting a high density of older stellar populations. Fainter, less-defined extensions surround the core, displaying a diffuse, reddish-orange hue which could indicate more evolved stars or the presence of dust. The galaxy does not appear to possess spiral arms or any distinct disk-like structure. There is a slight elongation in its shape, deviating from a perfect circle, which could suggest it is an oblate spheroid. No obvious signs of recent major mergers or strong tidal interactions are visible in the immediate vicinity of the galaxy. Faint color gradients are subtly present but there are no prominent star forming regions. The galaxy appears relatively isolated.
