The galaxy presents as a spiral galaxy, exhibiting distinct spiral arm structures. These arms appear relatively loosely wound. The central bulge of the galaxy is prominent and possesses a yellowish hue, potentially indicating an older stellar population. A disk is visible, but its orientation is tilted relative to our line of sight. The spiral arms are predominantly bluish, suggesting ongoing star formation. No signs of significant tidal disruption or interaction with neighboring galaxies are immediately apparent. The presence of a central bar could not be determined from this image.