The galaxy appears as a relatively smooth, elliptical structure with a concentrated central bulge. Its overall color is a yellowish-white, potentially indicating an older stellar population, although a slight blue tint in the core suggests some ongoing, albeit limited, star formation. The galaxy's light distribution is centrally concentrated, fading smoothly outward from the core, with no obvious spiral arm structure or dust lanes visible in this image. The ellipticity suggests the galaxy is not perfectly spherical, and may be slightly elongated. The smooth morphology suggests it is undisturbed, without evidence of recent major mergers or tidal interactions.
