The galaxy presents as a well-defined spiral structure with a prominent central bulge. The spiral arms are loosely wound and extended, displaying a discernible blue tint, suggesting active star formation regions populated with young, massive stars. The bulge appears yellowish-red, potentially indicating an older stellar population. Two major spiral arms are visible, originating from the core and extending outwards. There is a possibility of minor tidal distortions within the galactic disk, indicating a past or ongoing interaction. No strong bar structure is clearly visible.
