  In the lenticular galaxy NGC 1023 a new population of star clusters (``faint
fuzzies'') was recently discovered by Larsen & Brodie. These clusters are found
inside the disc and are faint (23 < V < 24 mag) and extended with effective
radii of r_eff approx. 7 to 15 pc. We present here N-body calculations of a
likely formation-scenario through merging star clusters in clusters of star
clusters (super-clusters). Such super-clusters are observed to form in
interacting galaxies. The resulting merger objects have masses comparable to
the ``faint fuzzies'' and show large effective radii (r_eff > 7 pc). Even
though these objects are suffering from strong tidal forces they are able to
survive and reach the estimated ages of the extended star clusters in NGC 1023.
