The galaxy presents as a relatively smooth, elliptical-like structure. The light profile appears centrally concentrated, with a gradual decrease in intensity outwards. The main body appears to be relatively undisturbed, without any obvious signs of major mergers or significant tidal features. A subtle asymmetry might be present but is difficult to characterize definitively. The overall color is consistent with an older stellar population, exhibiting a yellowish hue, indicative of evolved stars and potentially lower ongoing star formation activity. The apparent lack of prominent spiral arms or distinct disk structures further supports its classification as a spheroidal galaxy. Its estimated size suggests it's a moderate to large galaxy.
