NY Vir is a bright A-type star (about 0.46 solar masses, 32,780 K, 0.15 solar radii), 544 light-years from Earth. NY Vir b is a 2.66-Jupiter-mass companion, with an orbital period of 8.65 years, on an eccentric orbit (e ≈ 0.15), discovered in 2011 via eclipse timing variations. NY Vir c is a 5.54-Jupiter-mass companion, with an orbital period of 24.1 years, on an eccentric orbit (e ≈ 0.15), discovered in 2019 via eclipse timing variations. NY Vir adds another data point to the growing catalogue of planetary systems whose masses, orbits, and host-star properties constrain models of planet formation.