The galaxy presents as a somewhat face-on spiral, exhibiting a central bulge that appears moderately prominent and a distinctly flattened disk. Spiral arms are visible, though somewhat flocculent in appearance, tracing a loose and open pattern. The arms appear to be relatively symmetric. The central bulge displays a yellow-white hue, suggesting an older stellar population. The spiral arms exhibit a bluer color, indicative of ongoing star formation and the presence of younger, hotter stars. The galaxy appears well-defined, with a moderate degree of internal structure. There is no clear evidence of a strong bar structure. There is some observed disturbance within the morphology of this galaxy.
