The galaxy presents a disk morphology, viewed at a moderate inclination. The disk exhibits discernible spiral arm structure. These arms appear relatively tightly wound. The central bulge is prominent and of moderate size, exhibiting a yellowish hue suggesting an older stellar population. The disk shows bluer regions indicative of recent star formation along the spiral arms. A bar structure is possibly present, though not definitively strong. There are no obvious signs of major mergers or significant tidal disturbances.
