The galaxy presents a generally smooth, elliptical morphology. Its light profile appears concentrated towards the center, with a gradual decrease in intensity outwards. The central region exhibits a yellowish-white hue, suggesting an older stellar population. Moving outward, the galaxy displays a faint bluish halo. This halo indicates the presence of a younger stellar population, potentially ongoing, but low-level star formation. There is a subtle hint of a disk structure, although the galaxy appears predominantly spheroidal. No significant tidal features or signs of a major merger are readily apparent. The overall color suggests a mix of stellar ages, with the dominant population being evolved stars and a modest contribution from younger stars.
