The galaxy presents a spiral morphology, characterized by a well-defined, prominent central bulge. The arms are tightly wound around the bulge, and feature a yellow-white hue. The galaxy's disk appears relatively smooth, exhibiting a high degree of rotational symmetry with the spiral arms. The overall color suggests a population of older stars throughout the galactic body. The spiral structure is defined by areas of star formation. There is evidence of a bar structure dissecting the bulge of the galaxy. The galaxy's color and morphology suggests that it is relatively evolved, but may still have some ongoing star formation in localized regions within the spiral arms.
