The galaxy presents a largely smooth, elliptical morphology. The central region exhibits a concentrated, bright yellowish-white core, suggesting an older stellar population. Progressing outward from the center, the galaxy fades gradually. Subtle, diffuse, bluish extensions are observed along the edges of the central core. These suggest areas of fainter light. Overall, the galaxy appears relatively undisturbed, showing no major signs of tidal disruption or recent mergers. Its light profile appears highly concentrated with a strong central bulge.
