  In this paper we derive a possible mass profile for the low surface
brightness galaxy, Malin 1, based upon previously published space-based and
ground-based photometric properties and kinematics. We use properties of the
bulge, normal disk, outer extended disk and \ion{H}{1} mass as inputs into mass
profile models. We find that the dark matter halo model of Malin 1 is best
described by a halo profile that has undergone adiabatic contraction,
inconsistent with the findings for most disk galaxies to date, yet consistent
with rotation curve studies of M31. More importantly, we find that Malin 1 is
baryon dominated in its central regions out to a radius of $\sim10$ kpc (in the
bulge region). Low-surface brightness galaxies are often referred to as being
dark matter dominated at all radii. If this is the case, then Malin 1 would
seem to have characteristics similar to those of normal barred disk galaxies,
as suggested by other recent work. We also find that Malin 1 also falls on the
rotation curve shear versus spiral arm pitch angle relation for normal
galaxies, although more LSB galaxies need to be studied to determine if this is
typical.
