The galaxy appears as a somewhat elongated, diffuse object. It exhibits a distinct central region of higher surface brightness, suggesting a possible bulge or core. Fainter, extended structures surround this central region, potentially representing a disk component or tidal features. The overall color of the galaxy is bluish, which could indicate the presence of younger, hotter stars. The morphology appears to be somewhere between smooth and featuring some structure. Some irregularities are visible in the outer regions, possibly signifying minor disturbances. No clear signs of a major merger are immediately apparent, but subtle asymmetries could hint at past gravitational interactions.
