The galaxy appears to be a relatively smooth, elliptical or lenticular galaxy, displaying a concentrated central bulge that transitions into a more diffuse outer region. There is a slight hint of an extended disk-like structure, though it lacks prominent spiral arms. The galaxy exhibits a yellowish-orange hue, suggesting a population of older stars with lower rates of current star formation, potentially indicating an earlier type galaxy. The shape of the galaxy is somewhere between round and elliptical. There are no obvious signs of any significant ongoing merger activity or major disturbances to its morphology.
