The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. Its overall color appears to be yellowish-orange. This suggests a stellar population dominated by older, redder stars. The absence of prominent spiral arms or significant dust lanes indicates that it is likely an early-type galaxy. There is little to no visible evidence of ongoing star formation activity and the galaxy appears as a single, unperturbed object with a smooth luminosity profile, showing no signs of tidal tails, shells, or other features typically associated with recent mergers. 
