The galaxy presents as a relatively small, edge-on spiral with a prominent central bulge. The bulge exhibits a boxy shape with hints of a roundedness, and it appears to be the brightest region of the galaxy, displaying a strong yellow hue. This suggests an older stellar population dominating the bulge composition. The disk is thin and relatively smooth. A faint indication of dust lanes running along the midplane of the disk can be inferred. The overall morphology indicates a disk galaxy at a moderate redshift. There are no obvious signs of strong tidal distortions or major merger events.
