The galaxy appears to be a spiral galaxy, viewed at a slight angle. The central bulge is prominent and has a yellow hue, possibly indicating an older stellar population. The disk of the galaxy exhibits a bluish tint, hinting at the presence of younger, hotter stars within the spiral arms. Two distinct spiral arms are visible, tightly wound around the central bulge. The disk shows some patchy structure, with variations in color and brightness suggestive of star-forming regions. A strong central bar appears to extend through the center of the galaxy. The galaxy shows no major signs of a recent or ongoing merger, however, some minor disturbances are possible. Overall, the galaxy seems to be a well-defined spiral structure with ongoing star formation.