The galaxy presents as a luminous, relatively smooth object, likely an elliptical or lenticular type. Its shape appears moderately elliptical, showing a deviation from perfect circularity. There is a suggestion of a slight distortion or possible tidal feature, hinting at past or ongoing interactions, though the overall structure remains largely undisturbed. The galaxy exhibits a color gradient, becoming slightly redder towards its core. The light distribution suggests a centrally concentrated mass. No distinct spiral arm structures or prominent dust lanes are discernible. The galaxy's light profile appears smooth and diffuse, indicating an older stellar population and a low rate of current star formation.
