  We have analyzed the spatial distribution of galaxies from the release of the
Sloan Digital Sky Survey of galactic redshifts (SDSS DR7), applying the
complete correlation function (conditional density), two-point conditional
density (cylinder), and radial density methods. Our analysis demonstrates that
the conditional density has a power-law form for scales lengths 0.5-30 Mpc/h,
with the power-law corresponding to the fractal dimension D = 2.2+-0.2; for
scale lengths in excess of 30 Mpc/h, it enters an essentially flat regime, as
is expected for a uniform distribution of galaxies. However, in the analysis
applying the cylinder method, the power-law character with D = 2.0+-0.3
persists to scale lengths of 70 Mpc/h. The radial density method reveals
inhomogeneities in the spatial distribution of galaxies on scales of 200 Mpc/h
with a density contrast of two, confirming that translation invariance is
violated in the distribution of galaxies to 300 Mpc/h, with the sampling depth
of the SDSS galaxies being 600 Mpc/h.
