The galaxy presents as a spiral type, although the arms are somewhat difficult to discern in detail. The morphology appears to be that of a galaxy with flocculent spiral arms, the arms are not clearly defined. The galaxy is viewed at an angle, suggesting it may be close to edge-on. The central bulge appears prominent, with a high concentration of light, and the galaxy has an apparent size that indicates a fairly large stellar mass. There's a possibility of recent or ongoing interaction with a smaller galaxy.