The galaxy presents as a single, relatively smooth, and centrally concentrated object. It exhibits an elliptical morphology, appearing largely spheroidal with a slight deviation from perfect circularity. The light profile suggests a gradual decrease in intensity from the core outwards, indicating no pronounced spiral arm structures or a well-defined disk. The central region is a bright yellow, suggesting older stellar populations. There is a faint, diffuse halo extending beyond the main body, which gradually blends into the background. No obvious signs of tidal tails or significant morphological disturbances are apparent, suggesting that the galaxy may be a fairly relaxed system.
