The galaxy appears to be a spiral galaxy, observed at an intermediate angle, not quite edge-on.  Spiral arms are visible, possessing a somewhat clumpy structure, indicative of star forming regions. The galaxy exhibits a prominent bulge, but its size appears moderate relative to the disk. There is no obvious presence of a strong bar structure within the galaxy. The galaxy shows visual signs of a possible ongoing gravitational interaction or disturbance, possibly a minor merger. The central bulge appears somewhat yellow in color.  The disk is bluer than the bulge, indicative of younger stars.
