The galaxy presents as a relatively face-on spiral type, exhibiting a central bulge with spiral arms extending outwards. These spiral arms appear somewhat patchy and not clearly defined, with hints of blue indicating regions of active star formation. The overall color of the galaxy leans towards a bluer hue, suggesting a younger stellar population, especially in the arms. A slight dust lane is subtly visible, slightly obscuring some light from the core, adding to the galaxy's complex structure. The galaxy shows an apparent ellipticity, implying that it is not perfectly face-on, with one side appearing brighter than the other. There are possible minor disturbances in the outer regions, suggesting past interactions.
