The galaxy presents as a relatively smooth, elliptical structure. The central region exhibits a high concentration of light, appearing bright and slightly reddish in color, potentially indicating an older stellar population. A surrounding, more diffuse halo extends outwards, gradually decreasing in intensity. The overall shape is approximately round, with no apparent spiral arms or prominent disk features. There are no obvious signs of ongoing major mergers or significant tidal disturbances, although some minor irregularities in the outer halo cannot be ruled out at this resolution. The galaxy displays a color gradient, transitioning from redder hues in the core to slightly bluer tints in the outer regions. The overall morphology suggests a mature galaxy with a substantial spheroidal component.
