The galaxy presents as a centrally concentrated object with a relatively smooth morphology. It exhibits a discernible disk-like structure, with a slight elongation. There is an indication of spiral arm features, although they are not sharply defined. The central bulge is prominent and appears nearly spherical. The color profile suggests a mixture of stellar populations, with bluer hues in the disk indicating younger stars and ongoing star formation, contrasted by a possibly redder hue in the bulge representing older, more evolved stars. The galaxy displays no obvious signs of major interactions or significant disturbances. 
