The galaxy presents as a spiral galaxy viewed at an angle slightly inclined from face-on. It possesses well-defined spiral arms, exhibiting a moderate winding pattern. The central bulge appears relatively small and moderately luminous. The arm structure is somewhat flocculent. There appears to be a central bar present although it is not strongly pronounced. There is no strong evidence of a major ongoing merger although the galaxy is subtly asymmetrical. The color suggests the galaxy contains regions of active star formation. The galaxy does not exhibit a particularly smooth appearance, suggesting prominent disk features.