The galaxy appears as a single, relatively smooth structure with a concentrated central bulge and a faint, extended halo. The central region exhibits a yellowish hue, possibly indicative of an older stellar population. No distinct spiral arms or bar structures are readily apparent. The overall morphology suggests an elliptical or lenticular galaxy, appearing quite round. There is some evidence of disturbance on one side of the galaxy. The color gradients suggest varying stellar populations, possibly with ongoing, but relatively low, star formation. There are no indications of recent or major mergers.
