The galaxy presents as a smooth, relatively featureless elliptical morphology. It exhibits a centrally concentrated luminosity profile with a gradual decrease in brightness outwards, suggesting a high degree of radial symmetry. The galaxy's color index indicates a relatively old stellar population, with a noticeable absence of bright, blue star-forming regions. There is a subtle color gradient, where the central region exhibits a slight reddening compared to the outer halo. No obvious signs of spiral arms, bar structures, or tidal disturbances are visible. Overall, the galaxy appears as a well-relaxed system, possibly a massive galaxy with minimal ongoing star formation and no significant recent merger events.