The galaxy presents as a fairly smooth, elliptical object. It has a distinct orange hue. The core appears to be fairly concentrated. Based on the color, it is likely that the galaxy is comprised predominantly of older stars. There may be a very slight hint of a disk-like structure, but if present, it is minimal. There are no obvious signs of active star formation, such as blue regions or HII regions. The galaxy appears relatively undisturbed, showing no significant signs of tidal interactions or ongoing mergers.
