The galaxy presents a largely smooth, elliptical morphology. There is a concentration of light towards the center, appearing as a bright, yellowish core. A bluer hue surrounds the core, gradually fading into the background sky. The galaxy appears somewhat flattened, suggesting a degree of rotation, but does not exhibit prominent spiral arms or a distinct disk structure. The overall appearance is relatively undisturbed, showing no signs of major mergers or tidal interactions. The light profile suggests a centrally concentrated stellar population with a diminishing intensity towards the outer regions.
