The galaxy appears to be a spiral galaxy, observed at a significant redshift. The disk of the galaxy is tilted relative to our line of sight, presenting a somewhat edge-on view. There is evidence of spiral arm structure, although the arms are not sharply defined. The central bulge is prominent and appears yellow, likely indicating an older stellar population. The disk exhibits a bluer color, suggesting the presence of younger stars and ongoing star formation, especially on the far right side. There isn't any strong evidence of major merging activity or significant tidal disturbances, although there may be minor irregularities in the disk possibly suggesting a smaller interaction.
