J0155-4048: Lovell (1997) confirms the compact nature of the source on
6 km baselines, finding that 100% of the source flux density is contained
within an unresolved core component at 4.8 GHz. The source is mostly
resolved out on the shortest VLBA baselines (Fomalont et al. 2000).
Emission appears on both sides of the core, suggestive of a CSO
morphology, with the source extending over ~20 mas.