  We have obtained high resolution UV images with the HST+WFPC2 of the central
region of the dwarf elliptical galaxy NGC 205. Our images reveal that many of
the hot UV stars previously detected and studied from the ground are actually
multiple systems, open clusters and star associations. We have performed
photometry of two such clusters and we find our data are consistent with
stellar ages of 50 and 100 Myr, respectively. From the number of massive stars
in NGC 205 we estimate that the star formation episode in this galaxy has
turned ~1,000 Msolar of gas into stars over the last 100 Myr.
