The galaxy presents a smooth, elliptical morphology with a concentrated central bulge. The color profile indicates an older stellar population, with a dominant yellowish-orange hue. The light is fairly evenly distributed, suggesting no recent major mergers or active star formation in the past. Some minor disturbances are potentially present, based on some asymmetries. The overall shape is more in between round and elliptical. The galaxy exhibits a defined edge, suggesting its gravitational structure is fairly self-contained.
