The galaxy presents as an elongated, elliptical shape with a noticeable central bulge. The core exhibits a bright, relatively smooth appearance. Moving outwards from the center, the galaxy appears more diffuse with a softening of light intensity towards its edges. A slight bluing coloration in the central region suggests potential recent star formation. The overall structure appears relatively undisturbed, showing no obvious signs of major mergers, though minor disturbances cannot be ruled out. The smooth central region and the elongated form suggest a possible S0 or early-type spiral morphology.
