The galaxy presents a morphology consistent with a spiral galaxy, observed at a redshift of approximately 0.25. The galaxy exhibits distinct spiral arm structures, demonstrating a winding pattern that appears somewhat loose upon visual inspection. Two clear spiral arms are the dominant feature. A central bulge is apparent, but appears relatively small in comparison to the overall disk size, which contributes significantly to the galactic luminosity in the g, r, and z bands. There is evidence of a bar structure within the central region, extending across a considerable portion of the bulge. The disk is observed face-on. No major disturbances or signs of ongoing merger events are visibly apparent.
