The galaxy presents as a spiral, exhibiting a distinct disk-like structure. The spiral arms are readily apparent, winding moderately around a central bulge. The bulge appears somewhat prominent, giving the galaxy a classification leaning towards intermediate bulge size. Two spiral arms are observed. The bar structure is likely present, but is difficult to distinguish with certainty. The color distribution suggests ongoing star formation. There does not appear to be any major interaction or merging events. The galaxy disk appears to be nearly face-on from our perspective.
