The object presents as a spiral galaxy observed nearly edge-on. The central bulge appears prominent and elongated, with a smooth texture and a yellowish-orange hue, suggesting an older stellar population. The disk, viewed at a high inclination, is characterized by a diffuse, fainter light extending outwards from the bulge. There are no discernible spiral arm structures or distinct dust lanes visible, potentially obscured by the edge-on orientation and relatively high redshift of the galaxy. The overall morphology indicates a galaxy with a well-defined bulge component and a disk containing intermediate levels of star formation activity. There is no apparent evidence of tidal disturbances or interactions with other galaxies. The bulge appears rounded, exhibiting no clear boxy features. The general undisturbed appearance suggests the galaxy is not currently undergoing a major merging event.
