The galaxy presents a largely smooth morphology, with minimal indication of spiral arm structures or significant dust lanes. The central region exhibits a higher concentration of light, suggesting a prominent bulge component. The galaxy has a generally elliptical shape, tending toward roundness rather than a highly elongated form. There is no clear evidence of ongoing major merger activity or significant tidal disturbances, though minor irregularities cannot be ruled out. Color gradients within the galaxy suggest a stellar population that is slightly more evolved toward the center. The galaxy has a reddish color suggesting some ongoing star formation within the galaxy. 
