The galaxy presents a distinct spiral morphology. Two well-defined spiral arms emanate from a central bulge, exhibiting a moderate winding pattern. The arms are prominent and extend outwards from the bulge, suggesting ongoing star formation within them, and display a relatively flocculent structure. The galaxy does not appear to be edge-on; it is observed at an intermediate inclination angle relative to our line of sight. No signs of major mergers or significant tidal disturbances are apparent in the surrounding regions of the galaxy. The central bulge shows signs of older stellar populations, exhibiting a yellow hue. 
