  We present integrated photometry and color-magnitude diagrams (CMDs) for 24
star clusters in M33, of which 12 were previously uncataloged. These results
are based on Advanced Camera for Surveys observations from the Hubble Space
Telescope of two fields in M33. Our integrated V magnitudes and V-I colors for
the previously identified objects are in good agreement with published
photometry. We are able to estimate ages for 21 of these clusters using
features in the CMDs, including isochrone fitting to the main sequence turnoffs
for 17 of the clusters. Comparisons of these ages with the clusters' integrated
colors and magnitudes suggest that simple stellar population models perform
reasonably well in predicting these properties.
