The galaxy exhibits a distinct spiral structure. Two prominent spiral arms emanate from a central bulge. These arms appear relatively well-defined and feature a moderate winding, extending outwards from the core region. Within the spiral arms, there is evidence of star formation, indicated by the presence of bluer regions. The central bulge appears relatively moderate in size and displays a yellowish hue, suggesting an older stellar population. A bar structure is readily apparent and appears quite strong. The overall color profile suggests a mixture of stellar populations, with younger, bluer stars primarily located in the arms and older, redder stars concentrated in the bulge. The galaxy does not appear to be undergoing any major merging events, although some minor disturbances cannot be ruled out. The galaxy is observed face-on.
