We investigated global axisymmetric (m = 0) and nonaxisymmetric (m=1) modes of magnetic fields generated by the galactic dynamo including the α2-dynamo. The α2-dynamo is responsible for the field generation in the central region of galaxies where the shear of galactic rotation is weak (e.g. MS1). The highest growth rate of m= 1 modes is always smaller than that of m=0 modes; thus m= 1 modes of the standard galactic dynamo cannot explain the dominance of the bisymmetric fields in spiral galaxies. Radial extent of each m=1 mode is too narrow to reproduce the observed bisymmetric structure extending over a disk.
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