The galaxy presents as a relatively smooth, elliptical structure. The central region exhibits a bright, concentrated luminosity, suggesting a high density of stars. Moving outwards from the core, the light gradually diminishes. Some slight irregularities and faint extensions are apparent in the galaxy's outer regions; however, these do not indicate a major ongoing merger event, but may imply minor tidal disturbances. The overall color of the galaxy appears to be reddish-yellow, possibly indicative of an older stellar population with a reduced rate of active star formation, and indicative of an evolving, mature galaxy.
