The galaxy appears to be a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge that transitions outward to a fainter, diffuse halo. The overall color profile appears to be somewhat redder in the central regions, becoming slightly bluer in the outer halo, potentially indicating differing stellar populations. There may be some very subtle signs of minor tidal disturbance in the faint outer halo. The galaxy's morphology appears to be relatively undisturbed, with no obvious signs of a major ongoing merger or significant star formation within the galaxy. The galaxy is approximately round in shape.
