The galaxy presents an elliptical morphology, exhibiting a smooth, centrally concentrated light distribution. The core region appears bright and densely packed with stars, fading gradually towards the outer regions. A slight elongation is observed along its major axis, indicating a mild departure from perfect circularity. There is a subtle color gradient across the galaxy, with the central region appearing yellower and the outer halo appearing slightly bluer. This suggests a potential difference in stellar populations, with older stars dominating the core and younger stars more prevalent in the outskirts.
