The galaxy presents as a luminous, likely massive, object at a redshift of approximately 0.07. Its morphology appears predominantly smooth, with a high probability of being either smooth or exhibiting features consistent with a disk galaxy. The galaxy shows an intermediate ellipticity, neither perfectly round nor overly elongated, and shows no strong signs of recent or ongoing major merger activity. There is some possibility of minor disturbance present. The object exhibits strong absolute magnitudes in the g, r, and z bands. The galaxy appears to have an estimated stellar mass above 10^11 solar masses, and star formation is occurring. The galaxy is likely a later-type spiral, with the possibility of a central bulge.
