The galaxy presents as a relatively smooth, elliptical-like structure. Its core is intensely bright, yellow-white in color, suggesting a high concentration of older stars. The isophotes appear generally regular and without significant tidal features. There is a slight elongation to the galaxy's shape, with its light distribution extending further along one axis, though not dramatically. The color gradient changes gradually from the bright core to the dimmer outskirts, where there is evidence of a faint, blueish halo, possibly indicating the presence of a younger stellar population. Based on the apparent roundness, it seems to be observed at an intermediate inclination angle, as it is neither perfectly edge-on nor face-on. There are no prominent dust lanes or spiral arm structures visible, supporting its classification as an early-type galaxy. Faint disturbances might be present in the outer regions, but more detailed examination would be needed to confirm this.