This galaxy exhibits a well-defined spiral structure. The arms are prominent, displaying a characteristic winding pattern. A prominent bar feature bisects the central bulge, appearing robust and extends across a significant portion of the galaxy's diameter. The central bulge is moderately sized, exhibiting a smooth, concentrated luminosity that decreases outward. Dust lanes are subtly apparent within the spiral arms, contributing to the heterogeneous color profile. The galaxy shows no strong indications of major mergers or significant tidal disturbances, appearing relatively undisturbed. There appears to be a concentration of star formation in the spiral arms, which contributes to the blue color. 
