The galaxy appears to be a spiral galaxy, viewed at an oblique angle to its galactic plane. A prominent central bulge is evident, exhibiting a yellowish hue, which likely indicates an older stellar population. Fainter spiral arms extend outwards from the bulge. These arms have a bluer color compared to the bulge, implying more recent star formation. The galaxy's overall morphology suggests that it is relatively undisturbed and not undergoing any major mergers. The apparent size is consistent with a galaxy at intermediate redshift.
