The galaxy presents a largely smooth, elliptical morphology. Its color is predominantly yellow-orange, suggesting an older stellar population. The galaxy appears almost perfectly round in shape, with no discernible disk or spiral arm features. There are no obvious signs of a recent major merger, although a minor disturbance cannot be completely ruled out based on the available imagery. The galaxy appears relatively isolated in this field of view. The light is concentrated centrally, fading gradually outwards.
