The galaxy appears to be a relatively smooth, elliptical or lenticular system. It exhibits a centrally concentrated bulge, which is significantly brighter and more yellow-white in color. This region likely contains a high density of older stars. Extending outwards from the core is a more diffuse disk or halo, showing a bluer hue. This suggests the presence of a younger stellar population and possible ongoing, although modest, star formation activity. The galaxy's overall shape is somewhat elongated, deviating from a perfect sphere but not displaying strong spiral arm features. There are no obvious signs of major merger events or significant tidal disturbances, although subtle asymmetries or minor disturbances cannot be entirely ruled out with this data.
