The galaxy presents an elliptical morphology, appearing elongated with a smooth, diffuse light distribution. The central region exhibits a concentration of light, appearing brighter and more yellow. Moving outwards from the core, the galaxy exhibits a gradual decline in surface brightness. The outer regions appear less defined, fading into the background sky. Hints of bluer hues are observed in these outer portions. Overall, the galaxy's smooth appearance suggests a relatively evolved system. There are no prominent spiral arms or dust lanes visible in the image. The observed color gradient, from a yellowish core to bluer outskirts, suggests a possible radial variation in stellar populations.
