Аннотация:Fourier period analysis of our CCD observations taken from Oct. 26 till Nov. 1, 2008 (during the first 8 nights of the superoutburst), after trend removal, revealed the presence of small amplitude early superhumps (double-humped variations) with the period 76.46± 0.5 minutes (0d.0531). This period was used to construct the phase diagram of the residuals. Their mean values with errors are given in Fig. 4. The observations taken from Nov. 2 till Nov. 7, 2008 revealed the presence of 77.33±0.2 minutes (0d.0537) superhumps