The galaxy presents as a disk-shaped system viewed nearly edge-on. A prominent central bulge is observed, displaying a somewhat boxy morphology within the disk. The bulge exhibits a yellowish-orange hue, suggestive of an older stellar population. The disk itself is characterized by a bluer color, especially towards its outer regions, which may indicate ongoing star formation. Dust lanes appear to be present within the disk, obscuring some of the light from the central bulge. The galaxy appears relatively undisturbed, showing no strong evidence of a recent major merger, though some minor irregularities might exist. It is a fairly substantial galaxy, exhibiting characteristics of a spiral galaxy.
