We study galaxy correlations from samples extracted from the 2dFGRS final release .
Statistical properties are characterized by studying the nearest neighbor probability density , the conditional density and the reduced two-point correlation function .
The result is that the conditional density has a power-law behavior in redshift space described by an exponent \gamma = 0.8 \pm 0.2 in the interval from about 1 Mpc/h , the average distance between nearest galaxies , up to about 40 Mpc/h , corresponding to radius of the largest sphere contained in the samples .
These results are consistent with other studies of the conditional density and are useful to clarify the subtle role of finite-size effects on the determination of the two-point correlation function in redshift and real space .