The galaxy appears as a centrally concentrated, elliptical-like structure. It exhibits a smooth morphology with a high degree of radial symmetry. There is a bright, yellowish-white core that gradually fades into the surrounding halo. Faint blue colors are observed in the outer regions, possibly indicating some ongoing, albeit weak, star formation activity. No distinct spiral arms or bar structures are discernible. There are no apparent signs of major mergers or significant tidal disturbances. The galaxy appears relatively isolated and undisturbed.
