Morphology of void galaxies as a function of void-centric distance using other morphology catalogues. Morphology of void galaxies with respect to the normalised effective radius of the voids, similarly to Fig. 5, but considering the GZ1 morphology catalogue (upper panel), the GZ2 morphology catalogue (middle panel), and the CI parameter (lower panel). The dashed red vertical line represents the edge of the voids if they were spherical. Left panels: Relative number of early- (orange histograms) and late-type (blue histograms) void galaxies. Right: Fraction of early- and late-type galaxies, with their corresponding errors. Early-type galaxies are shown in orange and late-type galaxies in blue. Orange and blue dash-dotted horizontal lines indicate the mean fraction of early- and late-type galaxies using the corresponding morphology catalogue, while dotted horizontal lines indicate the mean fraction of early- and late-type galaxies using the DS18 morphology, 25.2% and 74.8%, respectively, for comparison. We use bins of 0.10 r/R_void. The fraction of early-type galaxies has been shifted by +0.01 r/R_void so that the error bars do not overlap.