The galaxy presents as a fairly smooth, elliptical-like structure. The light distribution is concentrated towards the center, indicating a dense nucleus. There is a slight color gradient, with the core appearing more yellowish-white, possibly indicating older stellar populations, while the outer regions exhibit a subtly bluer hue. There is no obvious indication of spiral arms or significant dust lanes. The galaxy appears undisturbed with no signs of ongoing major mergers or tidal tails. Overall, the galaxy seems to be a well-defined and relatively evolved system.
