The galaxy presents as a somewhat featureless, elliptical or lenticular galaxy with a smooth light distribution. It exhibits a centrally concentrated bulge which fades gradually into the outer regions of the galaxy. The shape appears moderately elongated, deviating slightly from a perfect circle. There is a subtle color gradient, with a yellower, presumably older stellar population concentrated towards the core, transitioning to a slightly bluer hue in the outer regions, which would indicate younger stars at a low star formation rate. No prominent spiral arms or dust lanes are visible, and there is no indication of any significant ongoing merger activity or major tidal disturbance.
