The galaxy presents as a largely smooth, elliptical or spheroidal structure. There's a highly concentrated central bulge that appears a warm, yellowish-orange, suggesting a population of older stars. A slightly bluer halo surrounds the core, indicating the possibility of some ongoing, though likely minimal, star formation in the outer regions. The galaxy is primarily round, though its shape could be described as slightly in between round and elliptical. No prominent spiral arms or distinct dust lanes are visible. There appear to be no signs of a major merging event or significant tidal disturbances.
