The galaxy presents a smooth, elliptical morphology, appearing largely featureless. There is a concentrated central bulge region exhibiting a yellow-orange hue, suggesting an older stellar population dominating the core. A more diffuse and slightly bluer halo surrounds the bulge, transitioning smoothly outward. There's little evidence of spiral arm structure or significant dust lanes within the image's resolution. The overall shape appears moderately elongated rather than perfectly spherical. The galaxy does not obviously display any signs of major ongoing merging activity.