This galaxy appears to be a spiral galaxy, observed at a redshift of approximately 0.08. The galaxy presents a disk-like structure with prominent spiral arms. There is evidence of tight winding in the spiral arms. The central bulge appears to be of moderate size, with some light distributed smoothly throughout. A weak bar-like structure may exist traversing the central region. Overall, the spiral arms are well-defined, suggesting a relatively undisturbed morphology, with no major signs of mergers or significant tidal disturbances. The color index suggests ongoing star formation, predominantly in the spiral arms.
