TOI-4507 is a Sun-like F-type star (about 1.11 solar masses, 6,260 K, 1.04 solar radii), 178 light-years from Earth. TOI-4507 b is a 0.06-Jupiter-mass companion, with an orbital period of 105 days, at 0.456 AU from its star, on an eccentric orbit (e ≈ 0.09), discovered in 2025 via transit. The planet was found when it crossed the face of its star, producing periodic dips in brightness that reveal its size and orbital period to space-based photometry. TOI-4507 b circles its star within the inner habitable zone.