The galaxy presents as a concentrated, centrally dominant bulge with a relatively smooth profile. There is some evidence of a faint disk structure extending from the central bulge, but the disk appears rather ill-defined. The overall color indices suggest a moderate population of young stars, yet the smoothness of the galaxy indicates that it has likely formed most of its stars already. There are slight irregularities observed that may indicate a minor gravitational interaction or past interaction. The morphological assessment implies it is a relatively evolved system without significant ongoing merging activity. The galaxy is situated at a considerable cosmological distance.
