Classification of the final catalogue of 1100 dwarf galaxy candidates. The darker shades on the outer circle correspond to the presence of the feature of interest. Left: nucleated fraction (outer circle) as a function of morphology (inner circle). Middle left: GC richness (outer circle) as a function of morphology (inner circle). Middle right: signs of disturbed morphology (outer circle) as a function of morphology (inner circle). Right: GC richness (outer circle) as a function of the nucleated fraction. A total of 1061 (96%) dwarf galaxy candidates are classified as dE (dI: 39 or 4%), 581 (53%) are nucleated, 282 (26%) are GC-rich, and 64 (6%) have a disturbed morphology.