The galaxy appears to be a spiral galaxy with a relatively bright, concentrated central bulge. Evidence of a disk structure is visible, although it seems somewhat disturbed, and potentially slightly warped. The galaxy displays a yellowish hue in the central region, possibly indicating an older stellar population, while the outer disk exhibits a bluer color, consistent with ongoing star formation activity. There's potential evidence of a minor interaction with a smaller companion galaxy, which may explain the disturbed morphology of the disk. The galaxy displays a intermediate specific star formation rate. Overall, the galaxy's morphology suggests a mass near 10^11 solar masses, with a star formation rate typical for galaxies of its mass at its redshift.
