The galaxy presents as a centrally concentrated spheroid of light with a notable lack of distinct spiral arm structures. Its overall shape is somewhat elliptical, deviating slightly from perfect circularity. There is a smooth, gradual decline in luminosity from the bright, unresolved core outwards. The color appears to be relatively uniform across the galaxy, with subtle color variations not easily discernable. The galaxy appears largely undisturbed, showing no prominent signs of tidal interactions or ongoing mergers. The smooth morphology suggests a higher fraction of older stellar populations. The general features observed indicate a high probability that this galaxy is classified as an elliptical galaxy. 
