The galaxy presents as a spiral galaxy, observed at an oblique angle relative to its galactic plane. The disk component exhibits a subtle, grainy texture suggestive of spiral arm structures, though these are not sharply defined. Blue hues are visible, concentrated primarily within the disk, indicating regions of active star formation. The central bulge appears somewhat prominent, exhibiting a smoother, more diffuse light profile, suggesting a concentration of older stellar populations. The galaxy shows a hint of a bar structure bisecting the central bulge. There are no obvious signs of major mergers or significant tidal disturbances. The overall morphology suggests a system with ongoing, but not necessarily intense, star formation within its spiral arms and a moderately sized bulge.
