The galaxy appears as a centrally concentrated, fairly smooth object. It exhibits a generally elliptical morphology, trending towards a more rounded shape. There is a color gradient visible, transitioning from a more yellow-white central region to a faint, slightly greenish outer halo. No distinct spiral arm structure or significant dust lanes are discernible. The overall structure appears relatively undisturbed, suggesting a lack of recent major merger events. Minor asymmetry in the outer halo might indicate a past minor interaction, but it is not pronounced. The faintness of the outer halo suggests a declining stellar density with increasing radius.
