The galaxy presents as a spiral type, with a prominent disk structure viewed at a relatively high inclination. The spiral arms are well-defined, exhibiting a loosely wound morphology and bifurcating clearly from the central region. A bar structure appears to be present within the central bulge, although the details are somewhat obscured. The bulge is moderate in size relative to the overall disk. There is a notable amount of blue light present in the spiral arms, suggesting ongoing star formation. The galaxy may be undergoing a minor interaction, as some slight distortion is visible in the disk morphology; but is possibly a normal spiral galaxy. The galaxy's disk demonstrates a relatively smooth appearance with two prominent arms.
