This galaxy appears to be a spiral galaxy, likely observed at a significant redshift. The central bulge is relatively bright and distinct, exhibiting a yellowish-orange hue suggesting a population of older stars. Faint spiral arms are possibly present, though the image resolution limits their clear identification. The overall light distribution appears elongated, indicating it is likely viewed at an angle. There appears to be some asymmetry in the galaxy's structure, possibly due to minor gravitational interactions with other galaxies. The blue color may suggest some regions of ongoing star formation activity within its structure.
