The galaxy presents a generally smooth, elliptical morphology. The core exhibits a concentrated, bright luminosity in the g and r bands, suggesting an older stellar population with ongoing star formation. The galaxy shows a radial decrease in surface brightness from the center outward. While the image resolution limits a definitive assessment, there is no obvious evidence of spiral arm structure, strong dust lanes, or a prominent disk. Some minor asymmetry is possibly present, but a major merger event is not indicated. The color profile indicates a redder central region that becomes bluer outward, consistent with star formation occuring in the outer regions of the galaxy. The general appearance suggests an elliptical galaxy with a substantial amount of mass, and moderate star formation.
