The galaxy presents an overall elliptical morphology. It exhibits a smooth, centralized light distribution, with a gradual decrease in luminosity from the core outwards. The color gradient suggests an older stellar population concentrated towards the center, with a yellowish hue. Moving outwards, the color shifts slightly towards redder tones, potentially indicative of a broader distribution of stars with varying ages. There's a subtle suggestion of a disk component or a slightly flattened structure, but it is not a dominant feature. No distinct spiral arms or significant dust lanes are apparent. There are no obvious signs of ongoing major merger activity or tidal disturbances, with the bulk of the galaxy undisturbed.
