The galaxy presents as a moderately bright, elliptical-shaped structure. Its core exhibits a concentrated, yellowish-white luminosity, suggestive of an older stellar population. The galaxy fades in intensity from its center outward, showing a gradual decrease in stellar density. There is a slight disk-like morphology with no well-defined spiral arms. The color gradients indicate possible regions of on-going, low star formation. Some minor disturbances are detected in the overall structure. 
