The galaxy presents a generally smooth morphology, appearing elliptical or lenticular in shape. The core is bright and concentrated, exhibiting a yellowish hue, suggesting an older stellar population. Fainter, bluer extensions surround the core, possibly indicating regions of more recent star formation, or interactions with a smaller galaxy. The overall structure seems relatively undisturbed, though subtle asymmetries hint at a past or ongoing minor interaction. The galaxy is relatively massive, and is thought to have a relatively low star formation rate.
