The galaxy presents as a spiral type, exhibiting a distinct disk structure with notable spiral arm features. Two primary spiral arms are clearly visible, emanating from a central bulge. The winding of these arms appears to be intermediate, not tightly wound nor completely open. The bulge size is moderate relative to the overall disk size. There is a hint of a bar-like structure, or rather a slight asymmetry to the bulge region, though it does not appear to be a strong, well-defined bar. There does not seem to be any major signs of ongoing or recent major merger events. Overall the galaxy demonstrates a somewhat clumpy morphology.
