The galaxy presents a clear spiral structure. The arms are well-defined, showing a relatively tightly wound configuration around a central bulge. A notable bar feature extends through the bulge region. The bulge itself appears to be of moderate size in relation to the disk. There's evidence of active star formation in the spiral arms, indicated by the presence of bluer regions. Overall, the galaxy appears as a relatively undisturbed system, showing no strong signs of ongoing or recent major merging activity, although some minor disturbances may be present in the arms or disk. The galaxy is observed at a significant redshift, suggesting a considerable distance.
