The arXiv preprint (abs/2605.24099) uses VLT/MUSE integral-field spectroscopy on two ultra-diffuse galaxies in the Fornax outskirts to measure low velocity dispersions, old (~10 Gyr) stellar populations, and overluminous globular clusters whose luminosity function mirrors the top-heavy distribution seen in NGC 1052-DF2/DF4. With a sample of just two systems and the acknowledged limitations of flattened mass estimators, the data favor a stars-only dynamical model over both cuspy and cored dark-matter halos. This configuration—75 kpc separation and 16 km/s relative velocity—represents a tighter present-day analogue than the 240 kpc, 358 km/s DF2/DF4 pair, implying the same exotic formation channel can yield observationally distinct endpoints. The bullet-dwarf collision model, first invoked for the NGC 1052 group, therefore gains indirect support from an independent environment, while the galaxies’ coeval GC and field-star ages align with predictions of a single high-velocity encounter ~10 Gyr ago. These findings intersect with documented LCDM tensions: the missing-satellites and too-big-to-fail problems, plus the unexpectedly high globular-cluster specific frequencies in some dwarfs. They also reopen discussion of modified-gravity alternatives that naturally suppress dark-matter content without fine-tuned baryonic feedback. Because the work remains a preprint, independent verification with deeper imaging or Jeans modeling is still required.