The galaxy presents as a spiral type, with a disk oriented close to face-on relative to our line of sight. Two dominant spiral arms are observed, exhibiting a grand design structure, although they appear somewhat flocculent. These arms wind outward from a central bulge, with an apparent intermediate size. The galaxy displays a hint of a central bar-like structure. Some knotty regions of star formation are evident within the spiral arms, with color variations suggesting the presence of both young, hot stars and older stellar populations. The disk is relatively thin and appears to be quite uniform in color. Overall, the system appears relatively undisturbed, showing no signs of major merger events or strong tidal interactions. The color suggests a late type spiral.