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The Im/dE,N mixed morphology dwarf ESO 359-G29 as a probe of a massive halo in NGC 1532

A low surface brightness dwarf, ESO 359-G29, in the neighborhood of the NGC 1532/31 pair, has the morphology of an early-type dE,N/dSO,N nucleated dwarf in yellow and red wavelengths, but shows an Sm or Im late-type morphology in the blue. This mixed morphology is similar to that of the prototype example NGC 4286, companion to NGC 4278. VLA observations of H I, however, show that ESO 359-G29 has a typical dwarf hydrogen content unlike NGC 4286 which is hydrogen depleted. The velocity distribution in NGC 1532 has also been determined from VLA observations of H I. At a distance of 64 kpc from the galaxy, the rotational velocity is 250 km s −1 , and it is still slowly increasing with distance