The galaxy exhibits an elliptical morphology, appearing as a smooth, elongated structure with a high degree of central concentration. It displays a color gradient, shifting from a yellowish-white core towards bluish outer regions. The central core suggests an older stellar population, while the bluer periphery may indicate the presence of younger, hotter stars or ongoing star formation. The galaxy does not show any signs of major disturbances, such as tidal tails or significant asymmetries, suggesting it is relatively undisturbed. There is a minor suggestion of a disk-like component, although the dominant feature is the smooth, elliptical shape. The object's overall appearance indicates a substantial stellar mass. The object is most likely quiescent, with a low specific star formation rate.
