The galaxy presents as a spiral type, with a disk-like structure that is not precisely edge-on, exhibiting a tilt that allows some view of the spiral arm structure. These arms are grand design, but not sharply defined. They exhibit a flocculent structure, appearing somewhat clumpy. There is a possible barred structure. The central bulge appears moderate. The color profile suggests active star formation, as evidenced by the blueish glow. The galaxy appears relatively isolated, showing no strong signs of tidal interactions or major mergers with other galaxies. There appears to be a minimal dust lane presence. The overall morphology suggests a system that has experienced, or is experiencing, ongoing, although not excessive, star formation. 
