Balmer H10 and H11 line profiles in the spectrum of EE Cep taken on 11 Aug. 2003 with an Echelle spectrograph on the 2.12 m telescope in SPM Observatory in Mexico. The best fit was obtained for a synthetic spectrum with: T_eff = 15   000 K, log g = 3.5,  [Fe/H]  = 0, and vsini = 350 km s^-1 (solid line). Two poorer fits calculated with different values of the rotational velocity, vsini = 300 km s^-1 (dashed line) and vsini = 400 km s^-1 (dash-dotted line), are shown for comparison purposes.