The galaxy presents a generally smooth and rounded morphology. It appears as a single, concentrated object with a central bulge. The light distribution is centrally peaked, exhibiting a smooth gradient decreasing outwards. The galaxy exhibits a yellowish hue at its center, transitioning to a redder color towards the periphery, which may indicate an aging stellar population in the outer regions. There is no visible spiral structure or dust lanes. No indications of ongoing mergers or major disturbances are present, although there may be very minor disturbances in the outer regions. The overall structure suggests an elliptical galaxy type.
