The galaxy presents as a disk galaxy, seen nearly edge-on. A prominent central bulge is visible, appearing smooth and somewhat concentrated. The bulge is characterized by a yellowish hue, suggesting a population of older stars. Fainter and bluer light extends along the galactic plane, indicating the presence of a disk component. Dust lanes are not clearly resolvable in this image, though some patchy obscuration may be present along the plane of the disk. Given the redshift, the galaxy is at a significant distance, resulting in a small angular size and limiting the resolution of finer details such as spiral arm structure or distinct star-forming regions. The overall morphology suggests a relatively mature galaxy with ongoing, but perhaps not exceptionally high, rates of star formation. There are no obvious signs of major mergers or tidal disturbances from this perspective.
