  We present 8 bright globular clusters and/or objects of less familiar nature
which we found in the course of scrutinizing the globular cluster system of NGC
1399. These objects are morphologically striking, either by their sizes or by
other structural properties. Some of them may be candidates for stripped dwarf
galaxy nuclei, emphasizing the possible role of accretion in the NGC 1399
cluster system. They are all highly interesting targets for further deep
spectroscopy or HST-imaging. Since these objects have been found within an area
of only 42 arcmin**2, we expect many more still to be detected in a full census
of the NGC 1399 cluster system.
