This galaxy presents as a disk-shaped structure, with a noticeable central bulge, although not sharply defined. A moderate degree of smoothness is observed across the galaxy's body, hinting at a well-mixed stellar population. Hints of spiral arm structures are present, but they are somewhat disrupted and lack well-defined edges. A blueish tint is observed across much of the galaxy, possibly indicating regions of active star formation. The galaxy is fairly isolated, showing no obvious signs of tidal interactions or major mergers in progress, although minor disturbances cannot be ruled out. The overall morphology suggests a galaxy transitioning between a spiral and a more lenticular state. 
