The galaxy presents as a relatively smooth, elliptical object. Its shape is somewhat elongated, appearing more cigar-shaped than perfectly round. A color gradient is visible, with the central region exhibiting a yellowish-white hue, potentially indicating an older stellar population. Fainter, bluer colors are present in the outer regions, which might suggest ongoing star formation. No distinct spiral arms or a prominent disk structure are observable; the light is diffuse and lacks sharp features. There are no obvious signs of major mergers or tidal disturbances in the main body of the galaxy.
