The galaxy presents a predominantly blue hue, indicative of ongoing star formation. It displays a spiral structure, though the arms appear tightly wound and somewhat ill-defined, potentially due to the viewing angle or image resolution. A central bulge is visible, appearing relatively small in proportion to the overall disk size. There is no apparent bar structure bisecting the bulge. The galaxy does not show any signs of major mergers, although some minor disturbances to its symmetry cannot be ruled out. Overall, the galaxy appears to be a late-type spiral galaxy with a moderate rate of star formation.
