The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits an elliptical morphology, appearing more oblate than perfectly spherical. There's a dominant bulge component evident by the concentration of light toward the center, which graduates into a fainter, more diffuse halo. I do not notice any distinct spiral arm structures. The overall color is slightly reddish or yellowish, indicative of an older stellar population. There may be regions of ongoing low-level star formation, as suggested by faint bluish areas in the outer regions. There are minor signs of disturbances, but there is no indication of a recent major merger. 
