The galaxy presents as a disk-shaped system viewed at a significant inclination. It exhibits a smooth, centrally concentrated light distribution, suggestive of a dominant bulge component. There is evidence of a faint, flattened disk extending beyond the central bulge. The color gradient shifts from a bluer hue in the central region to a redder tone in the outer regions of the disk. There are no immediately obvious spiral arm structures or significant dust lanes visible in this image. The galaxy appears relatively undisturbed.
