The galaxy presents as a moderately bright, elliptical-like structure with a high degree of central concentration. The core appears nearly spherical and exhibits a smooth luminosity profile, transitioning to a slightly more diffuse halo. The light distribution suggests a dominant bulge component. There is a subtle indication of a faint, disk-like structure surrounding the bulge. Its color is generally yellowish-white with hint of bluer regions, but appears mostly comprised of older stellar populations. Subtle asymmetries may indicate minor tidal interactions or internal disturbances. The size appears consistent with that of a typical galaxy in the local universe.
