The galaxy exhibits a spiral structure, with a prominent central bulge. The spiral arms are moderately wound, displaying a relatively ordered pattern extending outwards from the core. Two distinct spiral arms are clearly visible, originating near the central region and extending outwards.

The central bulge appears yellowish, suggesting an older stellar population. The spiral arms show variations in color, with bluer regions indicative of ongoing star formation and the presence of younger, hotter stars. The overall structure suggests a galaxy that is not undergoing any major merging events, although there might be minor disturbances in its overall symmetry.
