The results of photometric observations of seven E-type asteroids 64 Angelina, 214 Aschera, 1025 Riema, 1103 Sequoia, 1251 Hedera, 2035 Stearns, and 2248 Dwornik are presented. New rotation periods have been determined for asteroids 1025 Riema (6.557+/-0.001h), 1251 Hedera (15.015+/-0.010h), 2035 Stearns (85.0+/-0.1h), and 2048 Dwornik (3.664+/-0.001h). Two new poles have been estimated for 214 Aschera (274+/-8 o ; 64+/-4 o ) and 1025 Riema (141+/-10 o , 11+/-6 o ) and pole has been redefined for 64 Angelina (138+/-10 o , 31+/-5 o ). Using all available data on rotation periods, the spin rates of E-type asteroids have been analyzed. The distribution of the spin rates has maximum corresponding to the period of about 6.2h. The shapes of E-asteroids are more elongated than the shapes of small-size S-asteroids. The average values of color indexes, albedo and G parameter for E-type asteroids have also been determined.