Morphological classification of the 2674 dwarf galaxy candidates. Darker shades on the outer circle correspond to the presence of the feature of interest. Top left: Nucleated fraction (outer circle) as a function of morphology (inner circle). Top middle: GC richness (outer circle) as a function of morphology (inner circle). Top right: Signs of disturbed morphology (outer circle) as a function of morphology (inner circle). Bottom left: GC richness (outer circle) as a function of the nucleated fraction (inner circle). Bottom right: Blue-cored fraction (outer circle) as a function of the morphology fraction (inner circle). A total of 1548 (57.9%) dwarf galaxy candidates are classified as dE (dI: 1125 or 42.1%), 106 (4.0%) are nucleated, 26 (1.0%) are potentially GC-rich, 118 (4.4%) have a disturbed morphology, and 183 (6.9%) are blue-cored. It is important to note that the galaxies classified as disturbed were explicitly dEs; hence, there is no disturbed dI.