The galaxy presents a prominent spiral structure, appearing nearly face-on. It exhibits a well-defined, tightly wound spiral arm morphology. The arms originate from a relatively bright central bulge, which seems to be moderate in size. The color gradient suggests older stellar populations concentrated in the bulge, with the spiral arms displaying bluer hues, indicative of ongoing star formation. There is a hint of a bar structure running through the central region, which is quite pronounced. A noticeable amount of dust is seen along the spiral arms, especially along their inner edges. There appear to be multiple distinct spiral arms, approximately three to four, originating from the central region. No major signs of ongoing mergers or significant tidal disturbances are evident, though minor irregularities may be present in the outer arms.
