The galaxy presents an elliptical morphology, appearing largely smooth and featureless. It exhibits a concentrated central bulge, with a gradual decrease in luminosity extending outwards. The color profile suggests a relatively evolved stellar population, with a dominant redder hue. There is very little evidence of spiral arm structures or significant dust lanes. The shape is slightly elongated, without a high degree of flattening. The overall appearance suggests the galaxy is a massive, relatively quiescent system. There are subtle color gradients observable across the galactic body, implying variations in stellar populations or dust content. The faintness and small apparent size indicate the galaxy is at a substantial cosmological distance.
