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We present a first morphometric investigation of a preliminary sample fromthe SDSS of 154287 galaxies with apparent magnitude 14.5<m_r<17.5 and redshift0.001<z<0.4. We measure the Minkowski Functionals, which are a complete set ofmorphological descriptors. To account for the complicated wedge--like geometryof the present survey data, we construct isodensity contour surfaces from thegalaxy positions in redshift space and employ two complementary methods ofcomputing the Minkowski Functionals. We find that the observed MinkowskiFunctionals for SDSS galaxies are consistent with the prediction of aLambda--dominated spatially--flat Cold Dark Matter model with random--Gaussianinitial conditions, within the cosmic variance estimated from the correspondingmock catalogue. We expect that future releases of the SDSS survey will allow usto distinguish morphological differences in the galaxy distribution with regardto different morphological type and luminosity ranges.

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