The galaxy presents as a relatively smooth, elliptical morphology. There is a distinct central bulge that appears bright and concentrated. A fainter halo extends outwards from the core. The overall color is slightly blue, suggesting a component of younger stellar populations, although it's mostly dominated by older, redder stars. No prominent spiral arm structures or dust lanes are discernible. There is no visible indication of active galactic nuclei activity or any major mergers in progress, although subtle asymmetries might indicate past minor disturbances. The galaxy appears relatively isolated.
