Predicted MOND velocity dispersion for KK 197 as a function of its 3D separation to Cen A. The horizontal dashed lines show the MOND prediction (and its 1σ uncertainty) for the isolated case, while blue lines correspond to the MOND prediction considering the EFE from Cen A. The red dot is the measured value considering the stellar clusters. The 1σ and 2σ uncertainties are represented by the thick and thin red lines.