Some tantalizing points from the paper:
- They constrained the aspect ratio in two dimensions to be 10:1:C, but the third dimension is unconstrained. Depending on which axis the object is rotating around, C could either be 1, or 20. Either of these would be an essentially unique object within the solar system. This is a really weird shape.
- If the object is rotating around its short axis, it must have internal tensile strength (ie, it's a solid object, not just a pile of dust/gravel accreted by gravity). Lower bound on the required tensile strength is 3 Pascal (very little).
- There is essentially no dust/ice on the object - less than 1 kg within 2.5". So it's not a comet, and would have to be asteroidal. This conflicts with our current understanding of what objects would be in interstellar space. Current models have almost all objects ejected from our system being icy comets. This object would be analogous to a Manx comet, ie a rocky asteroid in a highly elliptical long period orbit.
- The shape of the observed light curve deviates from the best-fit triaxial ellipsoid in a way that suggests large flat or concave sections. It would take unrealistically large albedo variations to produce the same deviation without flat/concave sections.
And of course, of all the planets in the solar system, it made its closest approach to Earth, an astronomical "near miss" at just 0.16 AU :)