The galaxy exhibits a distinct spiral structure. The spiral arms appear prominent, extending outwards from a central bulge. The color distribution suggests a heterogeneous stellar population within the galaxy. The central bulge displays a yellowish hue, possibly indicating an older stellar population. Conversely, the spiral arms show bluer regions, which suggests ongoing star formation. 

The galaxy appears to be relatively undisturbed, showing no signs of major mergers. However, there may be a presence of minor disturbances or tidal interactions affecting its overall structure.
