The galaxy presents a largely smooth, elliptical morphology. There is a high concentration of light towards the center, suggesting a prominent bulge. The galaxy appears predominantly red, with a hint of green and blue light towards the edges. This potentially indicates a population of older stars with lower star formation activity throughout the galaxy's extended halo. There is no obvious evidence of spiral arms or a distinct disk. The light distribution appears relatively undisturbed, with no significant signs of tidal interactions or ongoing merger events, but there may be very minor asymmetries. The object is generally round in shape.
