The galaxy presents a largely smooth and elliptical morphology. Its color is predominantly yellow-orange, suggesting an older stellar population with a lower rate of ongoing star formation. The object appears relatively compact, exhibiting a high degree of central concentration. There is little evidence of spiral arms or significant disk features. The object is fairly symmetrical, displaying an approximately round shape with no signs of major disturbances or mergers. Minor asymmetries are not definitively ruled out given the resolution, but the overall structure implies relative quiescence.
