The galaxy presents as a single, relatively smooth object. Its color profile is dominated by a yellow-white hue at its center with a slight increase in redness as you move away from the center, suggesting a population of older stars and a low rate of current star formation. There is some indication of a slight elongation or flattening of the galactic disk, moving away from perfectly circular, as it appears to be an elliptical galaxy. There are no visible spiral arms or strong signs of recent mergers or tidal disturbances in the main body of the galaxy, though some faint, diffuse structure may be present in its outskirts, hinting at past interactions. The galaxy displays a relatively high degree of central concentration. It is likely a massive galaxy.