The galaxy presents a largely smooth, elliptical morphology. There is a concentrated, bright central bulge that appears yellow, suggesting an older stellar population dominates the core. A more diffuse halo surrounds this core, displaying a bluer hue, which could indicate ongoing or recent star formation activity in the outer regions. There's a general lack of distinct spiral arm structure or dust lanes. The overall shape of the galaxy is roughly circular, but there's a subtle elongation, deviating slightly from a perfect sphere. There is no obvious evidence of any major interactions or mergers. Minor disturbances cannot be ruled out.
