The galaxy presents as a single, luminous object with a generally smooth, elliptical morphology. There is a high degree of central concentration, with the brightest region appearing yellowish, possibly indicating an older stellar population dominating the core. Fainter extensions are noted, suggesting a degree of structure beyond a purely spherical distribution of stars. There is also a disk component that has features, though it appears somewhat smooth. No prominent spiral arms or dust lanes are discernible. Overall, the galaxy appears relatively undisturbed.
