The galaxy presents as a moderately inclined spiral, displaying a diffuse, almost hazy morphology. Its core region exhibits a concentration of light, suggesting a bulge component. Faint spiral arms are discernible, winding outward from the central region. Patches of bluer light are scattered throughout the disk, hinting at regions of active star formation. The overall color of the galaxy appears somewhat blue-shifted, indicative of ongoing stellar activity. Evident asymmetries in the structure may suggest gravitational interactions or a recent merger event.
