The galaxy presents as a somewhat faint, elongated structure with a moderate degree of smoothness. It is likely a disk galaxy seen at an angle. There is no definitive spiral arm structure visible, but rather a diffuse, oval-shaped central region that gently fades into the background sky. The color appears generally blue, suggesting the presence of younger stellar populations and ongoing star formation, though not at exceptionally high rates. There is no obvious evidence of major mergers or significant tidal distortions in its morphology. The galaxy exhibits some degree of central concentration, and it is slightly more luminous in the g-band than in the r and z bands. It appears to be fairly isolated, without any nearby companions or visible signs of interaction. It does not appear to be a spheroidal galaxy.
