  The power-law dependence of the angle in the angular projection of galaxy
distribution is explained by assuming that in the spherical shells within a
small angle the distributions are also fractal. If this local angular fractal
is possessed, a fractal structure is angularly-isotropic at each occupied point
though inhomogeneous, and is compatible with the present evidence claimed to be
of homogeneity for galaxy distribution. Further, it is most likely to be
isotropic rather than only angularly-isotropic. Several related issues are
discussed.
