The galaxy presents as a centrally concentrated object with a smooth, relatively featureless morphology. The light distribution appears largely elliptical, trending towards a rounded shape, showing a gradual decrease in luminosity from the core outward. The central region exhibits a strong orange hue, suggesting a population of older stars. The outer regions exhibit a subtle color gradient, trending towards slightly redder tones, consistent with aging stellar populations. There is no obvious spiral structure, disk component, or prominent dust lanes visible in this image. The overall structure appears relaxed, showing no signs of major merger activity or significant tidal disturbances.
