The galaxy presents as a disk-shaped system with a noticeable central bulge. It has a relatively smooth appearance, though some indications of structure exist within the disk. The disk exhibits a blueish tint suggestive of ongoing star formation, though the central bulge appears more yellowish, indicating an older stellar population. The galaxy appears somewhat elongated, with a suggestion of a faint, extended halo. There may be some minor distortion in the disk, though no major disturbances or merger events are clearly visible. Overall, the galaxy appears to be a relatively undisturbed spiral or lenticular galaxy undergoing moderate star formation.
