In this paper, we present UBVRI photometric results of SN 1994D which
covers the period from March 11 to April 4. All these data were obtain
ed with a Ford 2048x2048 CCD, which has been attached to the 60/90 cm
Schmidt telescope in Xinglong station, BAO. The light curves indicate
that the supernova is a normal type Ia, a good distance indicator of i
ts parent galaxy. The distance modulus of NGC 4526 is given as 30.07 /- 0.42.