Comparison of galaxy properties between the isolated and non-isolated subsamples of our parent dwarf sample. Left: M_⋆–M_H I relation. Isolated galaxies are plotted as purple squares, and non-isolated as orange circles. The error bars represent the median values and percentile errors, with the isolated sample shown as full purple lines, and non-isolated as dashed orange lines. The vertical black line denotes the stellar mass limit of 5 × 10⁹ M_⊙. Right: M_⋆–SFR relation. The markings are the same as in the left panel.