The galaxy presents a generally smooth, elliptical morphology. The light profile appears centrally concentrated, with a gradual decrease in surface brightness moving outward from the core. The color gradient indicates a population of older stars, particularly in the central bulge, with slightly bluer hues in the outer regions, suggestive of more recent, albeit subdued, star formation. There is no obvious spiral structure or dust lane. There is no obvious tidal disturbance. The galaxy's shape has moderate ellipticity.
