KMT-2023-BLG-2209L is a Sun-like G-type star (about 0.73 solar masses, 5,778 K), 5,570 light-years from Earth. KMT-2023-BLG-2209L b is a 0.80-Jupiter-mass companion, at 3.510 AU from its star, discovered in 2025 via microlensing. Microlensing detections occur when a foreground star's gravity briefly magnifies a background source, revealing planets that are otherwise too faint and distant to observe directly. KMT-2023-BLG-2209L b circles in the outer system, comparable to the Jupiter region. At roughly 5,570 light-years, KMT-2023-BLG-2209L lies far beyond the nearest stars yet remains reachable to large survey telescopes.