The galaxy presents a predominantly smooth morphology, with a notable central bulge that appears somewhat elongated. The light distribution suggests it is likely an elliptical galaxy. The outer regions exhibit a more diffuse, less structured halo of stars. There is a faint extension from the central region which may indicate some disk-like structure or tidal interaction. Overall, the galaxy is somewhat intermediate in shape, not perfectly spherical but not a highly flattened disk either. The color gradient suggests older stellar populations are dominant within the galaxy's main body, especially the central bulge. There are areas of blueish light, but they are less obvious. Any star formation occurring appears to be at a relatively low rate. No prominent dust lanes are observed, reinforcing the galaxy's evolved state. There may be a faint indication of a minor disturbance in its shape.