The galaxy presents as a relatively smooth, elliptical-like structure. The light distribution is concentrated towards the center, with a gradual decrease in luminosity towards the outer edges. The central region exhibits a yellowish hue, suggestive of an older stellar population. A subtle color gradient is observed, transitioning from a more yellow core to a slightly bluer halo, potentially indicating a small amount of ongoing or recent star formation in the outer regions. There are no obvious spiral arm structures or dust lanes visible within the image. No strong signs of any major mergers or significant tidal disturbances are present.
