The galaxy presents as a relatively smooth, centrally concentrated object. Its morphology appears largely elliptical, with an approximate radial symmetry. The color gradient transitions from a yellowish-orange core to a slightly bluer halo region. The galaxy exhibits minimal signs of spiral arm structure or significant dust lanes. There is no obvious evidence of recent major merger activity, tidal tails or strong gravitational distortions. The overall appearance suggests an evolved stellar population with limited ongoing star formation. The apparent size indicates it is a moderate galaxy in size. No notable fine structures or distinct features are readily apparent in the image.