The galaxy presents as a smooth, centrally concentrated object. Its morphology appears largely spheroidal, with little indication of a disk component or spiral arm structure. The light distribution is quite regular. The galaxy exhibits a gradual fading in intensity from the center outwards. There is a slight elongation along one axis, but the galaxy is generally round. The color is consistent with an older stellar population. No signs of significant ongoing star formation are readily apparent. There is no indication of recent major mergers or tidal disturbances affecting the galaxy's structure. Overall, it appears to be an elliptical galaxy.
