China’s Antarctic astronomical endeavors began at Kunlun Station, located at Dome A—the highest point of the Antarctic ice sheet—where survey telescopes such as CSTAR and AST3 have been deployed, achieving significant progress in fields such as exoplanet detection. To expand observational capabilities and leverage the unique advantages of different Antarctic sites, China has in recent years gradually developed optical astronomical facilities at Zhongshan Station, a coastal station. This paper presents a multi-functional astronomical observation system successfully constructed at Zhongshan Station during the 38th to 41st Chinese Antarctic Research Expeditions. The system comprises a wide-field photometric array of four 150 mm aperture telescopes, a 310 mm aperture rapid-tracking telescope, along with supporting automated observation platforms and a dome. During overwintering operation, a series of experiments—including accuracy calibration, detection frequency statistics, limiting magnitude verification, joint observations with domestic stations, and asteroid monitoring—were conducted. Field tests demonstrate that the system possesses high sensitivity for detecting faint targets and can achieve high-cadence monitoring of the same object by utilizing the continuous observation window available at high latitudes. The completion and routine operation of this system mark the establishment of a dual-station cooperative observation capacity in Antarctica, combining the deep-sky capabilities of Kunlun Station with the high-cadence, wide-field monitoring at Zhongshan Station. It provides a new experimental platform for frontier research in time-domain astronomy, near earth object surveillance, and related fields.