Comment by fatbird
This is, in fact, part of the support for Dark Matter, both with galaxies (the amount of lensing requires the galaxy to include a lot of Dark Matter) and between galaxies, where other lensing effects occur that can only be explained by filaments of Dark Matter between galaxies and galaxy clusters.
This is a great podcast, with episode 6 concentrating specifically on Dark Matter and the evidence for it: https://podcasts.apple.com/us/podcast/crash-course-pods-the-...
no. you can't say it's evidence for dark matter versus any given other theory until after you have computed the expected metrics created by any alternative theory.
in any case, you can't say it's support for dark matter in this specific case without actually running the numbers (what are the rotational speeds and what is the bending curvature)
dark matter halos must have a somewhat specific distribution that goes beyond the perimeter of the visible galaxy itself.
however the more that i think about it this example is likely to be unhelpful. the closer galaxy looks elliptical and most dense elliptical galaxies "have no dark matter" (in basic MOND this is a phenomenon that falls out if the gravity law). We'd really need lensing from a more "normal" looking galaxy.