  Strong cluster eccentricity evolution for $z \le 0.13$ has appeared in a
variety of observational data sets. We examine the evolution of eccentricity in
simulated galaxy clusters using a variety of simulation methodologies,
amplitude normalizations, and background cosmologies. We do not find find such
evolution for $z < 0.1$ in any of our simulation ensembles. We suggest a
systematic error in the form of a redshift-dependent selection effect in
cluster catalogs or missing physics in cluster simulations important enough to
modify the cluster morphology.
