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We present $UBVRI$ photometry for 392 star clusters and candidates in thefield of M33, which are selected from the most recent star cluster catalog. Inthis catalog, the authors listed star clusters' parameters such as clusterpositions, magnitudes and colors in the $UBVRIJHK_s$ filters, and so on.However, a large fraction of objects in this catalog do not have previouslypublished photometry. Photometry is performed using archival images from theLocal Group Galaxies Survey, which covers 0.8 deg$^2$ along the major axis ofM33. Detailed comparisons show that, in general, our photometry is consistentwith previous measurements. Positions (right ascension and declination) forsome clusters are corrected here. Combined with previous literature, weconstitute a large sample of M33 star clusters. Based on this cluster sample,we present some statistical results: none of the M33 youngest clusters ($\sim10^7$ yr) have masses approaching $10^5$ $M_{\odot}$; roughly half the starclusters are consistent with the $10^4$ to $10^5$ $M_{\odot}$ mass models; thecontinuous distribution of star clusters along the model line indicates thatM33 star clusters have been formed continuously from the epoch of the firststar cluster formation until recent times; there are $\sim 50$ star clusterswhich being overlapped with the Galactic globular clusters on the color-colordiagram, and these clusters are old globular clusters candidates in M33.

An updated catalog of M33 clusters and candidates: $UBVRI$ photometry, and some statistical results