The galaxy presents a discernible spiral structure. The arms are somewhat tightly wound, suggesting an intermediate stage of spiral morphology. There's a notable presence of active star formation within these spiral arms, indicated by their bluer hue. A well-defined central bulge is observed, displaying a more yellow/orange coloration compared to the spiral arms. The bulge appears of moderate size in relation to the overall galactic disk. The galaxy does not appear to be interacting or undergoing a major merger, but may be experiencing minor tidal disturbances. A strong bar structure crosses the central bulge.
