The galaxy appears to be a spiral galaxy, observed at a redshift of approximately 0.125. It is characterized by a distinct disk structure, with prominent spiral arms. The spiral arms are loosely wound and extend outwards from the central bulge, suggesting recent or ongoing star formation. The bulge appears relatively small compared to the overall size of the disk. The presence of a bar structure is evident, with a moderate concentration of light extending across the central region. Overall, the galaxy displays a vibrant blue hue, indicative of active star formation within its spiral arms. There appears to be no major merger event or significant disturbance of the structure.
