The 14 N͑p ជ, ␥͒ 15 O reaction has been investigated by measuring the angular distributions of its cross section and analyzing power using a 270-keV polarized proton beam. Calculations using a direct-capture-plusresonance model were compared with the data. The results indicate the presence of ␥ transition amplitudes which were not considered in previous extrapolations of the astrophysical S factor to low energies. The impact on the zero-energy S factor of the 14 N͑p ជ, ␥͒ 15 O reaction is discussed.