  We present a quantitative study of the morphology of 41 Extremely Red Objects
(EROs). The analysis is based on deep otical and near-infrared images from the
Hubble Space Telescope public archive, and performed by fitting to each galaxy
image a PSF-convolved bi-dimensional model brightness distribution. Relying
both on the visual inspection of the data and on the results of the fitting
procedure, we are able to determine the fraction of irregular and/or
interacting EROs, and to identify those that more closely resemble local
ellipticals. To the former class, whose members are probably high-redshift
dusty starburst, belongs about 15% of the whole sample, whereas the
elliptical-like objects are between 50 and 80% of the total. A few galaxies,
although characterized by a compact morphology, are best fitted by an
exponential distribution, more typical of local spirals. Our data also suggest
that irregular EROs are found predominantly in the field, and that - on average
- they tend to be characterized by the reddest colors. Finally, we plot the
rest-frame Kormendy Relation ($\mu_e$ vs. $R_e$) for a sample of 6 EROs with
spectroscopic redshifts ($z \sim 1.3$), and estimate its evolution with respect
to the local relation.
