The galaxy presents as a centrally concentrated, luminous spheroid. Its overall shape is relatively smooth and appears undisturbed. There is a slight elongation observable, but it is generally round. The central region exhibits a strong, yellowish-white luminosity, indicative of a substantial population of older stars. The light gradually fades toward the outer regions of the galaxy. There is no indication of spiral arms or a prominent disk structure. Minor disturbances cannot be completely ruled out, but this object gives the appearance of being an elliptical galaxy.
