This galaxy exhibits a spiral structure, with visible arms extending from a central bulge. The arms appear somewhat loosely wound and asymmetric, indicating possible past or ongoing interactions. The central bulge appears moderate in size, and is a yellow-white hue, suggesting an older stellar population. Star formation is likely occurring within the spiral arms, as evidenced by the presence of bluish regions that indicate younger, hotter stars. Overall, the galaxy presents a mixed morphology, suggesting a complex evolutionary history. Its redshift indicates that the light from this galaxy has been traveling for a significant portion of the universe's age.
