jats:titleAbstract</jats:title> jats:pDark-matter-deficient galaxies (DMDGs) discovered in the survey of ultra-diffuse galaxies (UDGs), in apparent conflict with standard cold dark matter, may be produced by high-velocity galaxy–galaxy collisions, the so-called Mini-Bullet scenario. Recent observations of an aligned trail of 7–11 UDGs near NGC 1052, including DMDGs DF2 and DF4, suggesting a common formation event, ∼8.9 ± 1.5 Gyr ago, provide a test.Hydro/jats:italicN</jats:italic>-body simulations, supplemented by galaxy orbit integrations, demonstrate that satellite–satellite collisions outside the host-galaxy virial radius can reproduce the observed UDGs in the NGC 1052 group. A trail of ∼10 DMDGs is shown to form, including 2 massive ones that replicate the observed motions of DF2 and DF4. The linear relation, jats:bold jats:italicv</jats:italic> </jats:bold> = jats:italicA</jats:italic> jats:bold jats:italicx</jats:italic> </jats:bold> + jats:bold jats:italicv</jats:italic> </jats:bold> jats:sub0</jats:sub>, conjectured previously to relate positions (jats:bold jats:italicx</jats:italic> </jats:bold>) and velocities (jats:bold jats:italicv</jats:italic> </jats:bold>) of the aligned DMDGs as a signature of the collision event, is approximately obeyed, but individual DMDGs can deviate significantly from it. The progenitors whose collision spawned the trail of DMDGs survive the collision without themselves becoming DMDGs. We predict that one progenitor is located at the end of the trail, which can be tested by observing the difference between its stars, formed pre-collision, from those of the DMDGs, formed post-collision. By contrast, stellar ages and metallicities of the DMDGs are nearly identical. We further offer a hint that the tidal field of host NGC 1052 may contribute to making DMDGs diffuse. ΛCDM simulation in a 100 cMpc box finds our required initial conditions ∼10 times at jats:italicz</jats:italic> < 3. These results indicate current observations are consistent with the Mini-Bullet scenario.</jats:p>