The object presents as a lenticular or early-type spiral galaxy at a redshift of approximately 0.17. It exhibits a dominant, smooth, and somewhat elongated spheroid component, consistent with an elliptical or S0 morphology. The galaxy's color profile suggests an older stellar population, as indicated by the reddish-yellow hue. There is no discernible spiral arm structure or significant dust lane obscuration visible in this image. The galaxy appears relatively isolated, without any obvious signs of ongoing major merger activity or tidal disturbances, although minor asymmetries or disturbances cannot be completely ruled out. The spatial extent of the galaxy is relatively compact. Overall, the galaxy appears to be a relatively massive, passively evolving system.
