The galaxy presents as an edge-on spiral, exhibiting a clear disk structure. The dust lane bisecting the galaxy is prominent and relatively uniform, suggesting a well-established and relatively undisturbed disk. The bulge appears smooth and rounded, contributing to a centralized luminosity gradient. There are no obvious signs of recent major mergers or significant tidal disturbances in its morphology. There is a slight hint of some disturbances occurring. The disk has a faint blue/green tint implying some star formation but given the bulge color, the galaxy is mostly comprised of older stars.
