The galaxy presents a somewhat flattened, elliptical appearance. Its overall structure suggests a disk galaxy, but the bulge dominates its luminosity. The central region exhibits a yellow-orange hue, indicating an older stellar population likely concentrated within the bulge. Moving outward from the center, a bluer component is visible within the disk, suggestive of more recent star formation. The disk displays some signs of disturbances, but without strong indications of recent major merger events. The galaxy is not perfectly round but more elliptical, with no dominant spiral arms.
