This galaxy presents as an elliptical morphology, lacking prominent spiral arm structures. It exhibits a smooth, centrally concentrated light profile, with the luminosity decreasing gradually outwards from the core. The galaxy appears largely spheroidal in shape, with a modest amount of ellipticity. Color gradients are subtle; the central region appears slightly more yellow, potentially indicating an older stellar population relative to the outer regions which appear slightly bluer. There is no obvious evidence of a recent major merger event or significant tidal disturbances based on the smooth light distribution and symmetrical structure. However, there may be minor disturbances in the light distribution. The galaxy seems to be relatively quiescent in its star formation activity based on the color.
