The galaxy presents as a barred spiral structure, although the spiral arms appear somewhat flocculent and not as tightly wound. The bar structure itself is prominent, spanning a significant fraction of the galaxy's diameter. There is evidence of active star formation within the arms, exhibited by a bluer color. The central bulge is moderately sized. There appears to be an indication of minor tidal disturbances or interactions based on the slight asymmetry in the outer regions of the galaxy and the relatively diffuse nature of the surrounding halo. Overall, the galaxy appears to be an actively star-forming system with a prominent bar and indications of ongoing or recent interactions.
