The object presents as a spiral galaxy, observed at an oblique angle relative to its plane. Evident spiral arm structures extend from the central bulge. The arms display a tightly wound morphology, suggesting a relatively high shear rate within the galactic disk. Star formation regions are visible as subtle, localized concentrations of bluer light within these arms. The central bulge appears moderately sized, with a mild concentration of light. There is some indication of a central bar-like structure. Overall, the galaxy appears relatively undisturbed, with no obvious signs of major merger activity, although some minor irregularities in the disk are noted.
