The galaxy presents a smooth, elliptical morphology with a high degree of central concentration. It appears largely featureless, lacking prominent spiral arms or a distinct disk structure. The galaxy's shape is neither perfectly spherical nor highly elongated, exhibiting an intermediate axis ratio. There is no evidence of significant tidal disturbances or ongoing major mergers. The galaxy exhibits a subtle color gradient, appearing slightly bluer towards the outer regions and redder towards the core. This may indicate ongoing, though relatively low, levels of star formation activity, concentrated in the outer regions, or a population of younger, bluer stars in the periphery. No signs of active galactic nuclei are apparent.
