The galaxy presents as a disk galaxy, exhibiting a significant disk component. A central bulge is apparent, with a moderate size relative to the overall galaxy. Faint spiral arm structures are suggested within the disk, though not sharply defined. The galaxy is viewed at an oblique angle, not quite edge-on or face-on. Evidence for a bar structure is present, although it is not particularly prominent. No obvious signs of major mergers or significant disturbances are observed, although a minor disturbance cannot be ruled out. Overall, the galaxy appears to be a relatively normal spiral galaxy.
