The galaxy presents as a fairly smooth, elliptical structure. Its light profile appears centrally concentrated with a gradual decrease in intensity outward, indicative of an older stellar population. It possesses a generally rounded morphology and lacks any obvious signs of spiral arms or bar features. There is no significant dust lane apparent across the major axis. The galaxy's color seems to be concentrated towards the redder end of the spectrum which is consistent with the lack of recent or ongoing star formation. The overall appearance suggests this is a relatively evolved, quiescent galaxy, potentially an elliptical galaxy. No signs of a major merging event or significant tidal disturbances are immediately apparent, which supports the idea of a relatively relaxed system.
