The galaxy presents a spiral morphology with tightly wound arms. A central bulge is evident, exhibiting a yellowish hue, suggestive of an older stellar population. The spiral arms appear bluish, indicating the presence of younger, hotter stars. Dust lanes appear subtly interspersed within the arms, obscuring some of the starlight. The galaxy displays a high degree of rotational symmetry. The galaxy's overall shape appears close to circular. No obvious signs of a major ongoing merger are discernible.
