The galaxy presents as a spiral type, observed at an inclined angle relative to our line of sight. It exhibits a prominent central bulge that appears bright and yellowish. The spiral arms are well-defined, tightly wound, and trace a distinct pattern around the bulge. The galaxy's disk appears relatively thin and shows evidence of active star formation regions, indicated by blueish hints along the spiral arms. Overall, the galaxy's structure shows a dominant bulge and spiral arms, without evidence of any major disturbances or merging events.
