The galaxy appears to be an elliptical galaxy, exhibiting a largely smooth and featureless morphology. Its overall shape approximates a sphere, with only a slight deviation towards an elongated form. The central region displays a high concentration of light, which gradually diminishes towards the outer edges of the galaxy. The color profile indicates a dominance of older stellar populations, as evidenced by the redder hues observed, although bluer colors are also present. There is no clear indication of spiral arms or a prominent disk structure, which supports the classification as an elliptical galaxy. Minimal signs of recent merging events or significant tidal disturbances are observable. The galaxy's relatively compact size suggests a mature system that has undergone significant evolutionary processes.
