The galaxy presents a generally smooth, elliptical morphology. The core is very bright and concentrated. There is a noticeable color gradient, with the central region exhibiting a more yellow/white hue, suggesting an older stellar population. The outer regions are less luminous, appearing slightly redder in color. Overall, the galaxy exhibits a high degree of symmetry. No spiral arm structures or significant dust lanes are visible. The galaxy's light is highly concentrated towards the center, and it has a relatively high Sersic index, suggesting a high concentration of stars towards the center. Based on the light profile, it is most likely a massive galaxy with little recent star formation.
