The galaxy presents as a centrally concentrated system with a smooth, featureless morphology. Its color profile suggests a dominant stellar population of intermediate to older age. The galaxy exhibits a near-circular symmetry, showing no obvious signs of tidal interactions or major morphological disturbances; however, there may be minor disturbances. The concentration of light towards the center indicates the likely presence of an elliptical galaxy. Based on its color and morphology, star formation is likely low.
