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We present our new photometry of DV Psc obtained in 2010 and 2011, and newspectroscopic observation on Feb. 14, 2012. During our observations, threeflare-like events might be detected firstly in one period on DV Psc. The flarerate of DV Psc is about 0.017 flares per hour. Using Wilson-Devinney program,we derived the preliminary starspot parameters. Moreover, the magnetic cycle is9.26(+/-0.78) year analyzed by variabilities of Max.I - Max.II.

Photometric study of the short-period RS CVn eclipsing binary DV Psc