  This paper is the third which examines galaxy morphology from the point of
view of comprehensive de Vaucouleurs revised Hubble-Sandage (CVRHS)
classification, a variation on the original de Vaucouleurs classification
volume that accounts for finer details of galactic structure, including lenses,
nuclear structures, embedded disks, boxy and disky components, and other
features. The classification is applied to the EFIGI sample, a well-defined set
of nearby galaxies which were previously examined by Baillard et al. and de
Lapparent et al. The survey is focussed on statistics of features, and brings
attention to exceptional examples of some morphologies, such as skewed bars,
blue bar ansae, bar-outer pseudoring misalignment, extremely elongated inner SB
rings, outer rings and lenses, and other features that are likely relevant to
galactic secular evolution and internal dynamics. The possibility of using
these classifications as a training set for automated classification algorithms
is also discussed.
