The galaxy presents as a relatively smooth, elliptical or lenticular structure. It exhibits a centrally concentrated bulge region which appears yellow-white in color, suggesting a population of older stars. There is a subtle gradient in color from the center outwards, with the outer regions appearing slightly bluer, possibly indicating a small amount of ongoing or recent star formation. No prominent spiral arms or bar features are discernible. There is only minor evidence of tidal disturbances or mergers, though some slight asymmetry may be present. Overall, the galaxy appears as a fairly evolved system with a dominant spheroidal component.
