The galaxy presents as a flattened, elliptical shape viewed nearly edge-on. There is a prominent central bulge that appears relatively smooth and concentrated. The disk is elongated and exhibits a reddish hue along its major axis, suggesting an older stellar population or significant dust obscuration. Fainter, bluer regions are observed tracing along the edge of the galaxy, indicating areas of more recent star formation activity. There are no indications of strong spiral arm structures, however some faint features are visible that are close to the galactic plane. The outer regions of the galaxy exhibit a gradual fading, with the galactic plane showing some defined edges. Overall, the galaxy's morphology suggests a relatively evolved system.
