The galaxy presents as a relatively smooth, elliptical-like structure. The light is concentrated towards the center, indicating a prominent bulge. There's a color gradient from the core to the outer regions, with the central region exhibiting a yellowish-white hue suggesting an older stellar population, while the outer regions appear slightly bluer, potentially indicating younger stars, although the overall blue fraction is low. There is no evidence of spiral arms or prominent dust lanes. The galaxy appears isolated and unperturbed, showing no signs of tidal interactions or recent mergers. The overall morphology indicates a galaxy with a substantial spheroid component. The apparent roundness suggests it is likely an elliptical galaxy viewed with its major axis close to the plane of the sky.
