The galaxy appears to be a spiral galaxy, presented face-on to our line of sight. It has a bright, yellowish central bulge. Surrounding the bulge are prominent spiral arms, exhibiting a flocculent structure. The spiral arms are relatively tightly wound near the central bulge but somewhat loosely wound overall. The arms display a bluish hue, suggesting the presence of ongoing star formation within them. The outer regions of the disk appear somewhat disturbed, hinting at possible interactions or minor mergers in the galaxy's past. The galaxy shows evidence of a bar structure crossing the central bulge, albeit a subtle one. The color gradients across the galaxy suggest variations in stellar populations and dust content. There is a hint of dust lanes near the central regions. Overall, the galaxy presents a complex morphology typical of actively star-forming spiral galaxies at a redshift of approximately 0.0777.
