The galaxy presents a primarily face-on orientation. A discernible disk structure exhibits spiral arm features; these arms are somewhat flocculent in nature. The central region displays a moderate bulge component that appears relatively smooth and centrally concentrated. Overall, the galaxy's luminosity appears moderate, indicating a galaxy of intermediate size and mass. There is no obvious evidence of a strong bar structure. There does appear to be minor asymmetry present in the spiral arm structure. Further analysis of color gradients may indicate active star formation regions.
