The galaxy presents as a relatively smooth, lens-shaped structure. It has a prominent central bulge that appears yellowish-white in color, suggesting an older stellar population. The disk component appears somewhat flattened and extends outwards from the central bulge, showing a bluer hue hinting at the presence of some younger stars.  There's a very faint, diffuse halo surrounding the brighter central regions. There is no obvious spiral structure visible, nor any signs of major disturbances or ongoing mergers. Its morphology suggests a galaxy transitioning from a spiral type toward a lenticular or elliptical.
