The galaxy presents as a spiral, exhibiting a slight disk-like morphology. The bulge is moderately prominent, and the spiral arms appear somewhat flocculent and not tightly wound. There appears to be some irregularity in the structure, and the galaxy appears to be of intermediate ellipticity. No obvious major merger features are evident, though there may be some minor disturbance. Based on the colors, it appears that some level of star formation is occurring.
