  We recently discovered that NGC 3201 has characteristics that set it outside
the current twofold classification scheme for Galactic globular clusters (GCs).
Most GCs are mono-metallic and show light-element abundance variations (e.g.,
Na-O and C-N anti-correlations); but a minority of clusters also present
variations in Fe correlating with s-process element and C+N+O abundances, and
they possess multiple C-N sequences. These anomalous GCs also have a broad
sub-giant branch (SGB) and follow the same mass-size relation as dwarf galaxies
possibly evolving into GCs. We now revealed that NGC 3201 belongs to neither
group. It has multiple C-N sequences, but no broad SGB, no strong evidence of a
Fe-spread, and it does not follow the mass-size relation.
