This galaxy appears to be a relatively smooth, elliptical system. The light profile indicates a concentrated central bulge that gradually fades into a more diffuse halo. There is a slight color gradient, with the core exhibiting a yellowish hue, potentially indicating an older stellar population dominated by redder stars. Fainter, slightly bluer regions extend from the central core, potentially indicating some amount of recent star formation, although it appears largely quiescent. No spiral arm structures or strong dust lanes are immediately apparent. The overall roundness and lack of significant distortions suggests this galaxy has not undergone any recent major mergers, or that any past interactions have since relaxed into its current smooth morphology. Evidence suggests it is a relatively massive galaxy.
