The galaxy presents as a spiral galaxy with a moderate bulge. The spiral arms are tightly wound and exhibit some degree of patchiness, suggesting ongoing star formation activity. The disk appears inclined to our line of sight. Evidence of a bar structure is present, though its strength appears moderate. There are no clear signs of major mergers or significant tidal disturbances affecting the galaxy's morphology. The galaxy is generally blue, but a bit more red in the central area near the bulge.
