The galaxy presents as a somewhat elliptical, smoothly distributed light source. The central region exhibits a concentration of brighter, yellowish light, suggesting a higher density of older stellar populations. Progressing outward from this center, the light appears slightly more diffuse, with a faint bluish-white hue noticeable on the edges. The galaxy appears relatively undisturbed, with no obvious signs of spiral arm structure or major mergers. Subtle irregularities in the outer regions are consistent with either a faint disk structure viewed at an angle, or only minor disturbances. The galaxy is not perfectly spherical, presenting a slightly elongated shape.
