The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. There is a subtle gradient in color, shifting from a slightly bluer hue in the outer regions to a more yellowish-white core, suggesting a variation in stellar populations. The overall shape exhibits a degree of ellipticity, appearing somewhat flattened rather than perfectly spherical. No distinct spiral arms or significant dust lanes are discernible within the resolution of the image. There is no obvious sign of any tidal debris or other external disturbances, which would suggest a relatively isolated system without recent major merger events.
