The galaxy presents as a spiral type, observed at an oblique angle, but not fully edge-on. Distinct spiral arms are visible. The winding of these arms appears relatively tight. A prominent bar structure is evident across the central region of the galaxy. The bulge component appears to be moderate in size relative to the disk, but not so prominent as to be large or dominant. The disk component is the primary visible structure. There is no obvious major merger, although a minor disturbance cannot be ruled out. The overall color index suggests the presence of both younger, bluer stars in the spiral arms and older, redder populations within the bulge and perhaps the bar. The size appears to be of average.