The galaxy presents as a relatively smooth, elliptical shape with a noticeable central bulge. It exhibits a generally uniform color gradient, transitioning from a brighter, yellower core to a slightly bluer outer region. There is an indication of a minor disturbance or possible interaction, inferred from the asymmetry in the outer halo. The light distribution suggests an evolved stellar population with ongoing, though perhaps diminished, star formation. Overall, the galaxy appears to be in a late-stage of its evolution with characteristics of both an elliptical galaxy and a weak disk galaxy.
