The galaxy presents a distinct spiral morphology. The spiral arms are prominent and loosely wound. The galaxy exhibits a notable central bulge, though not overwhelmingly dominant. There may be a weak bar structure present. The color distribution suggests ongoing star formation within the spiral arms, evidenced by bluer hues. There are no obvious signs of major mergers or significant tidal disturbances, though the galaxy may be experiencing minor interactions. The galaxy is not seen edge-on. The nucleus appears active, or with higher concentration of older stars which indicates possible central black hole activity.
