The galaxy presents as a relatively smooth, elliptical-like structure. There is little evidence of spiral arms or significant disk features. The light profile appears centrally concentrated, with a gradual decrease in luminosity towards the outer regions. The galaxy displays a color gradient, transitioning from a yellowish-white core to a more reddish hue in its outer regions. This suggests a possible difference in stellar populations, with older, redder stars dominating the outer halo and younger, bluer stars concentrated towards the center. There appear to be no obvious signs of recent or ongoing major mergers, though there may be slight irregularities in the outer contours indicating minor disturbances. Overall, the galaxy seems to be an evolved system, likely a relatively massive galaxy with moderate star formation.
