The galaxy appears as a single, relatively smooth object with a near circular morphology. A notable color gradient is visible, shifting from a reddish core to a greenish outer region. The core exhibits a higher surface brightness, suggesting a concentration of older stellar populations. The outer region, while fainter, displays a bluer hue, possibly indicating ongoing or recent star formation activity. There is no obvious spiral structure or distinct dust lanes. A slight asymmetry or minor disturbance is weakly suggested by subtle unevenness in the outer halo. The overall light distribution indicates an elliptical or lenticular type galaxy.
