Complete CCD light curves of the Algol-type eclipsing binary IU Persei have been obtained in the B, V, R and I filters during 7 nights in 2006 with the 40-cm telescope of the Gerostathopoulion Observatory of the University of Athens. The light curves are analyzed with the W-D program in order to determine the geometrical and photometric elements of the system. Moreover, the outside eclipses light variations have been used for searching of pulsating component(s) in the system.