The observed galaxy appears to be a relatively smooth, elliptical-type galaxy. It exhibits a concentrated central bulge which is bright yellow in color. The galaxy has a well-defined core which quickly fades into a dimmer, less saturated corona. The shape of the galaxy tends toward a rounded form, with only slight elongation. No apparent spiral arms, dust lanes, or signs of active star formation are discernible. There is no evidence of any major tidal disturbances or ongoing merging events. The galaxy's structure indicates it is a system that has undergone significant dynamical relaxation and quiescence.
