The galaxy presents as an elliptical structure with a smooth, centralized concentration of light. The core region exhibits a bright, yellowish-white hue, indicating a likely concentration of older stellar populations. Moving outward from the core, a gradual decrease in luminosity is observed, transitioning into a less defined and slightly bluer halo. The overall shape appears moderately elongated. There may be some evidence of a faint, extended disk-like structure or tidal features, but this is difficult to confirm based on the image. The color gradient suggests a potential decline in star formation from the inner regions to the outer regions. There are no obvious signs of strong spiral arms or a prominent dust lane.
