The galaxy presents as a relatively smooth, elliptical morphology with a concentrated central bulge. The light distribution suggests a high degree of symmetry around the galactic center. There is a subtle color gradient, transitioning from a yellowish-white core to a bluish halo. No distinct spiral arm structures or dust lanes are visible within the galaxy's body. The overall color profile indicates a mature stellar population with a possible presence of recent star formation towards the outer regions, as suggested by the bluer light. There is no evident sign of tidal disturbances or ongoing mergers. The galaxy appears relatively isolated and undisturbed.
