The galaxy presents a largely smooth, elliptical morphology, with a high degree of central concentration. The core exhibits a yellowish-orange hue, suggesting an older stellar population. The outer regions appear slightly bluer in comparison, hinting at the presence of some younger stars or ongoing, albeit subdued, star formation. Overall, the galaxy appears relatively isolated, with no immediately apparent signs of major tidal interactions or ongoing mergers. There might be faint indication of a slight asymmetry or minor perturbation in the outer envelope, but further investigation is needed to determine this more precisely. The observed light profile is fairly regular and not significantly elongated, as it is close to being circular.
