The galaxy presents a distinct spiral morphology. The central bulge appears relatively small and moderately bright with a yellowish hue, potentially indicating an older stellar population. The spiral arms are tightly wound and extend outwards from the central bulge. There seems to be a high number of spiral arms, but it is hard to tell. These arms are characterized by a bluer color, which is indicative of ongoing star formation. No bar structure is clearly visible within the central region. The galaxy is seen face-on, offering a comprehensive view of its spiral structure. There is no evidence of significant merger activity or major tidal disturbances. Overall, this galaxy is likely a spiral galaxy with a prominent disk and a relatively quiescent bulge region.
