The galaxy presents an elliptical morphology, appearing elongated in shape. The central region exhibits a high concentration of light, indicative of an older stellar population, possibly a bulge. The color gradient transitions from a yellowish core to a bluer halo, suggesting the presence of more recent star formation in the outer regions, but it's mostly smooth. There's some asymmetry in the outer halo with a small hint of a disk-like structure. No apparent tidal features or obvious signs of major merger activity are visible. The overall structure suggests a relatively evolved system undergoing moderate star formation.
