The galaxy appears to be a relatively large and luminous system, exhibiting a flattened, elongated morphology reminiscent of a disk galaxy, though lacking clear spiral arm structures. It exhibits a dominant central bulge region appearing smooth in texture and has a yellowish-orange hue, possibly indicative of an older stellar population with lower ongoing star formation activity within the core. The outer regions present bluer tinges, possibly implying ongoing star formation in the galactic disk. The main body has a smooth appearance and a majority fraction, suggesting a lack of significant disturbances or interactions, although a slight asymmetry in the disk's brightness distribution cannot be ruled out. The morphology also exhibits a notable elongation. This object has a noticeable red hue, pointing to a high redshift.
