The observed galaxy presents a clear spiral morphology. Tight spiral arms emanate from a central bulge, displaying a relatively high degree of winding. The bulge appears moderately sized, with a yellow hue indicative of an older stellar population. A prominent bar structure traverses the galactic center, appearing rather strong and well-defined. The disk component shows complex structure, with some regions exhibiting bluer colors suggestive of ongoing star formation. There are hints of minor disturbances or asymmetries within the spiral arms, possibly indicating past interactions. The galaxy is presented at a face-on orientation, affording a clear view of its spiral structure.
