The galaxy presents as a relatively smooth and centrally concentrated object. Its morphology is largely spheroidal. The light profile appears quite uniform, lacking any distinct spiral arm structures or a prominent central bar. The galaxy exhibits a subtle color gradient, with a core that has a slightly yellow hue, transitioning to a bluer halo. There are no visible tidal features or other signs of recent major merger activity. Its overall appearance is indicative of a system that is relatively undisturbed, with a large fraction of its stellar population likely composed of older stars. The absence of obvious dust lanes further supports this assessment. The light distribution is dominated by a smooth component, likely a stellar bulge. The galaxy's profile suggests a mature system, possibly an elliptical or lenticular galaxy.
