  We present the structural parameters of $\sim910$ dwarf elliptical-like
galaxies in the local universe ($z\lesssim0.01$) derived from the $r-$band
images of the Sloan Digital Sky Survey (SDSS). We examine the dependence of
structural parameters on the morphological types (dS0, dE,dE$_{bc}$, dSph, and
dE$_{blue}$). There is a significant difference in the structural parameters
among the five sub-types if we properly treat the light excess due to
nucleation in dSph and dE galaxies. The mean surface brightness within the
effective radius ($<\mu_{e}>$) of dSph galaxies is also clearly different from
that of other sub-types. The frequency of disk features such as spiral arms
depends on the morphology of dwarf galaxies. The most pronounced difference
between dSph galaxies and other sub-types of early-type dwarf galaxies is the
absence of disk feature which is thought to be closely related to their origin.
