The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge, characterized by a bright, diffuse glow that appears yellowish-white in color. The surrounding disk region shows a gradual decrease in surface brightness with increasing radial distance from the center. The disk appears to be tilted with respect to our line of sight, giving it an oval shape. Some slight asymmetry can be seen in the outer regions, which may indicate minor disturbances. There does not appear to be much evidence of active star formation or distinct spiral arm structure. Overall, the galaxy appears to be a mature system with a prominent bulge and a smooth disk.
