The galaxy presents as a centrally concentrated, diffuse object, likely an elliptical galaxy at a redshift of approximately 0.17. The primary light distribution is relatively smooth with no distinct spiral arm structures or pronounced dust lanes visible. The galaxy appears to be fairly massive, exhibiting a significant absolute magnitude across the observed g, r, and z bands. Star formation appears to be low but not negligible, and there is a potential for minor gravitational disturbance possibly indicating an interaction with another galaxy in the past. Overall, it has a fairly symmetrical, intermediate-rounded shape and shows no obvious signs of a recent major merger. The galaxy appears to be dominated by an older stellar population.
