relatively recent development of wide-field imaging and spectroscopy that we have been able to substantially increase the sample of known GCs in [NGC 5128]{}. Despite these difficulties, the return on these investigations has the potential to be large — [NGC 5128]{} is the only large elliptical whose stellar populations can be studied in detail, and its proximity makes it the local benchmark for studies of more distant early-type galaxies.

A [*UBVRI*]{} Broadband\
Imaging Survey of NGC 5128
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Observations
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[cccllllll]{} CTR & 13:25:30 & $-$43:01:33 & $37.6\times38.6$ & 3600 & 1500 & 1800 & 1000 & 1000\
& & & & 1.20 & 1.27 & 1.25 & 1.24 & 1.18\
NE & 13:26:46 & $-$42:28:25 & $36.0\times38.1$ & $3719^{b}$ & 1500 & 1800 & 1800 & 1500\
& & & & 1.38 & 1.32 & 1.21 & 1.04 & 1.26\
S & 13:25:27 & $-$43:26:30 & $37.2\times39.1$ & $3662^{b}$ & 1500 & 1800 & 1800 & $1608^{b}$\
& & & & 1.26 & 1.12 & 0.96 & 1.11 & 1.97\

We conducted our imaging survey with the Mosaic II optical CCD camera on the Blanco 4-meter telescope at Cerro Tololo Inter-American observatory (CTIO). We observed three fields with Mosaic 