This galaxy exhibits a prominent spiral structure. There are multiple spiral arms emanating from a bright, concentrated central bulge. The winding of the spiral arms appears to be intermediate, neither tightly wound nor loosely defined. The bluer color of the arms suggests ongoing star formation within these regions. The galaxy is viewed face-on. There may be evidence of some minor interaction or disturbance in the overall morphology, although a merger is not immediately obvious. The central bulge contributes significantly to the galaxy's overall luminosity. The lack of a clearly defined bar feature is also worth noting. The distribution of light appears relatively smooth when transitioning from the bulge outwards into the disk.
