The galaxy presents as a generally smooth, elliptical-like structure with a concentrated central bulge. The light distribution is relatively uniform, with a gradual decrease in intensity from the center outwards. There is a subtle color gradient, shifting from a yellow-white core to a slightly redder periphery. No distinct spiral arm structures or dust lanes are apparent. The overall impression is that of a well-defined, mature galaxy with a high degree of symmetry. There may be slight disturbances in the smooth light distribution, possibly suggesting a very minor interaction or merger event in its past. The galaxy appears relatively isolated, with no obvious companion galaxies in close proximity.
