The galaxy presents a largely smooth, elliptical morphology. The light distribution is concentrated toward the center, displaying a bright core region. Moving outwards from this nucleus, the light profile smoothly decreases in intensity. There is little evidence of spiral arm structure or dust lanes. The galaxy exhibits a color gradient, shifting from a yellowish-white central region to more reddish hues in the outer areas, possibly indicating an older stellar population in those regions. The overall shape deviates slightly from a perfect circle, appearing somewhat elongated but not highly flattened. There are no obvious signs of recent or ongoing major merger activity. Minor disturbances may be present, but are not strongly evident. The apparent size on the sky is relatively small.