The galaxy appears to be a relatively smooth, centrally concentrated object, likely an elliptical or lenticular galaxy. Its overall shape is generally round, exhibiting a high degree of circular symmetry. There is a bright, prominent central bulge that dominates the galaxy's luminosity profile. Moving outward from the center, the light gradually fades. There is some evidence of minor disturbance or asymmetry in the galaxy's outer regions. There seems to be a concentration of light separate from the main body of the galaxy. This may indicate an ongoing or past interaction. The color suggests an older stellar population, lacking substantial recent star formation. Overall, the galaxy presents as a relatively undisturbed, evolved system.
