The galaxy presents a largely smooth, elliptical morphology with a high degree of central concentration. The core exhibits a bright, yellowish hue, suggesting an older stellar population likely dominated by red giant stars. The overall structure is generally round, showing minimal signs of a disk-like structure or spiral arms. There is a subtle color gradient extending outward from the core, with the outer regions appearing slightly bluer, perhaps indicating the presence of a younger, albeit still subdued, stellar population at the galaxy's edges. No prominent dust lanes, tidal tails, or signs of recent major mergers are evident. Faint, diffuse light extends beyond the immediate core region, indicating the presence of a surrounding halo of stars. The galaxy appears relatively undisturbed and quiescent, with no indications of active star formation.
