The galaxy presents as a relatively bright, disk-shaped structure, observed at an oblique angle, displaying characteristics suggestive of a spiral or lenticular galaxy. The central region exhibits a bright, concentrated bulge. A fainter, extended disk surrounds the bulge. The disk's color is more blue than the bulge. The galaxy appears to have moderate star formation activity, concentrated in the disk, as suggested by the bluer colors. There may be some minor disturbance or interaction noticeable in the outer disk, though a merger event is not evident.
