The galaxy appears to be a relatively smooth, elliptical or lenticular type galaxy, exhibiting a moderate redshift. It possesses a generally round morphology, with a color gradient suggesting older stellar populations. There's a slight hint of some sort of possible disturbance, though it doesn't suggest a major merger event, possibly a minor interaction or internal asymmetry. The overall luminosity indicates a relatively massive galaxy. Based on its color and morphology, the galaxy's star formation rate is likely low, indicative of a more evolved system where star formation has largely ceased.
