  A detailed analysis of the galaxy distribution in the Southern Sky Redshift
Survey (SSRS) by means of the multifractal or scaling formalism is presented.
It is shown that galaxies cluster in different ways according to their
morphological type as well as their size. Ellipticals are more clustered than
spirals, even at scales up to 15 h$^{-1}$ Mpc, whereas no clear segregation
between early and late spirals is found. It is also shown that smaller galaxies
distribute more homogeneously than larger galaxies.
