The galaxy presents a smooth, elliptical morphology, appearing largely featureless. It exhibits a high degree of roundness in its overall shape. The light distribution is concentrated toward the center, with a gradual decrease in intensity toward the outer edges. The primary color is a yellowish hue, indicating an older stellar population, with some redder regions possibly indicating dust presence. The absence of distinct spiral arms or prominent star-forming regions suggests a relatively quiescent galaxy with a low star formation rate. There is no visible evidence of on-going major mergers. The presence of minor disturbances cannot be ruled out. The object appears as a single, relatively undisturbed system.
