The galaxy presents as an elliptical morphology with a smooth, centrally concentrated light distribution. The core appears bright and yellowish-white, indicating a concentration of older stellar populations. The overall shape is elongated, with a major axis that is roughly three times the length of its minor axis. The outer regions of the galaxy exhibit a gradual fading of light intensity and a more reddish hue, suggesting a decline in star formation activity towards the periphery. No distinct spiral arms or dust lanes are discernible. The galaxy appears relatively isolated, showing no obvious signs of tidal interactions or recent mergers.
