The galaxy presents as a largely featureless elliptical type with a high degree of central concentration. The core exhibits a yellowish-orange hue, suggesting an older stellar population. A diffuse greenish halo surrounds the central region, possibly indicative of ionized gas emission or a population of younger, hotter stars at the galaxy's periphery, though this could be due to the blending of different bands of light. The overall morphology appears smooth and undisturbed, with no obvious signs of recent major mergers or tidal interactions. The galaxy’s shape appears mostly round, with little indication of elongation or a disk-like structure.
