The galaxy presents as a somewhat flocculent spiral, displaying spiral arm structures. The arms appear loosely wound and are not as clearly defined or tightly packed. There is a suggestion of ongoing star formation within these arms, indicated by subtle blueish regions along their length, although precise locations of star-forming regions are difficult to discern at this resolution.

A prominent central bulge is observable, appearing moderately sized in relation to the overall galactic disk. The bulge exhibits a yellowish hue, suggestive of an older stellar population. No bar structure is clearly visible traversing the galactic center, but the image resolution limits definitive confirmation.

The overall colour of the disk is a blend, appearing mostly red, suggesting a mix of stellar populations, with the red perhaps implying a more dominant aging stellar population. There also appears to be signs of minor disturbance or interaction, but no obvious merger or collision with another large galactic structure.
