The galaxy appears as a moderately luminous, disk-shaped system, oriented nearly edge-on from our perspective. A central bulge is clearly visible, exhibiting a brighter, yellowish hue compared to the surrounding disk. The disk itself shows some evidence of structure, but lacks the distinct spiral arms characteristic of grand design galaxies. The disk appears relatively smooth and somewhat diffuse, suggesting a moderate degree of star formation activity. The shape of the galaxy is rather elongated, with the major axis significantly larger than the minor axis. The lack of significant dust lanes or prominent HII regions further suggests that this galaxy is in a later stage of evolution. Overall, it presents as a typical spiral galaxy at a moderate redshift, displaying a mix of evolved stellar populations and ongoing star formation. The galaxy's visual morphology is consistent with an intermediate Hubble type. There are some hints of slight asymmetry, potentially suggesting a past or ongoing minor interaction with another galaxy, although no clear companion is immediately obvious.
