The galaxy presents as a face-on spiral, exhibiting a prominent central bulge with a bright nucleus. Spiral arms are visible, although somewhat flocculent and not sharply defined. The arms display a patchy distribution of star formation regions, with some evidence of HII regions exhibiting a bluer hue. The overall color gradient suggests a higher concentration of older stellar populations in the bulge region, transitioning to younger, bluer stars in the spiral arms. There is no visual indication of a strong bar structure bisecting the galaxy, nor are there any obvious signs of a major ongoing merger event or significant tidal distortions. There is a hint of a disk component to the galaxy that is mostly unobscured, and does not appear to be seen completely edge on.
