The galaxy presents a largely elliptical morphology. It appears relatively smooth and exhibits a radial concentration of luminosity towards the center. The central region is bright, with a yellowish-white color, indicating an older stellar population. The outer regions appear fainter and slightly more reddish, suggesting the presence of dust or a slightly younger stellar population compared to the core. There is no clear evidence of spiral arms or significant disk-like structures. The galaxy appears relatively undisturbed, lacking any obvious signs of major mergers or tidal interactions. A very subtle elongation is possibly present, giving it an in-between roundness, however, overall, it appears largely circular from our line of sight.
