The galaxy presents as a spiral galaxy, exhibiting a clear disk structure. The spiral arms appear somewhat loosely wound and are visible, though not sharply defined. There's a prominent central bulge that is bright and concentrated. Dust lanes are hinted at within the disk, obscuring some of the starlight, but they are not prominent. The galaxy displays a general bluish hue in the spiral arms, suggestive of ongoing star formation, while the central bulge appears more yellow, indicating an older stellar population. There might be a hint of a bar-like structure across the center of the galaxy but that is not very obvious. Overall, the galaxy seems fairly isolated, without any obvious major signs of tidal disruption, though some minor disturbance cannot be ruled out.
