The galaxy presents as a centrally concentrated, elliptical-like object with a smooth light distribution. The central region exhibits a pronounced, diffuse luminosity, appearing almost spheroidal, suggestive of a bulge. The overall color profile transitions from a yellowish-orange core to a bluer halo, hinting at varying stellar populations. The absence of distinct spiral arms or prominent dust lanes suggests a relatively evolved system. There is a very slight asymmetry to the galaxy. There is no obvious indication of a significant ongoing merger event.