The galaxy presents as a moderately luminous, elliptical-like structure at a redshift of approximately 0.168. Its overall form appears relatively smooth, with a centrally concentrated bulge region that emits strongly across the observed g, r, and z bands, suggesting an older stellar population. The galaxy exhibits a slightly elongated shape, showing neither a defined disk nor spiral arm structures. There are no obvious tidal features or signs of recent major merger events. The general morphology indicates a galaxy with a substantial stellar mass and a modest rate of star formation. Observed colors suggest a red sequence galaxy with predominantly evolved stellar populations, with only marginal blue light indicating slight recent star formation. The effective radius appears to be approximately 5.6 kpc, which is consistent with an intermediate to massive galaxy.
