The galaxy presents as an elliptical-type galaxy at a redshift of approximately 0.18, based on photometric redshift estimations. It exhibits a smooth, largely featureless morphology with a high degree of central concentration. The galaxy appears nearly circular, showing minimal ellipticity. There is no apparent evidence of spiral arm structures or prominent dust lanes.

Color gradients are subtle, with a slightly redder core region transitioning to a somewhat bluer halo or outer envelope. This color variation potentially indicates a difference in stellar populations, where the core may be dominated by older, redder stars, while the outer regions may have a younger, bluer population, possibly indicative of ongoing or recent star formation at a low rate. The galaxy does not show signs of significant interaction or merging activity, exhibiting a relatively undisturbed structure. 
