This galaxy exhibits a distinct spiral morphology. The arms are prominent and extend noticeably from the central bulge region. There appears to be at least two main spiral arms that are relatively tightly wound. The color distribution across the galaxy suggests active star formation, particularly within the spiral arms, and a more quiescent stellar population in the central bulge. There's no indication of a major merger event in the recent past, but perhaps minor disturbances. The galaxy is observed at a redshift which indicates it is at a significant distance from us. The core of the galaxy is bright and yellow while the spiral arms are tinted blue, indicating a difference in age between the population of stars in these regions.