  We present the first large-scale stellar kinematic and line-strength maps for
dwarf elliptical galaxies (9 in the Virgo Cluster and 3 in the field
environment) obtained with the SAURON integral-field unit. No two galaxies in
our sample are alike: we see that the level of rotation is not tied to
flattening (we have, e.g. round rotators and flattened nonrotators); we observe
kinematic twists in 1 Virgo and 1 field object; we discover large-scale
kinematically-decoupled components in 2 field galaxies; we see varying
gradients in line-strength maps, from nearly flat to strongly peaked in the
center. The great variety of morphological, kinematic, and stellar population
parameters seen in our data points to a formation scenario in which properties
are shaped stochastically. A combined effect of ram-pressure stripping and
galaxy harassment is the most probable explanation. We show the need for a
comprehensive analysis of kinematic, dynamical, and stellar population
properties which will enable us to place dwarf ellipticals and processes that
govern their evolution in the wider context of galaxy formation.
