The galaxy presents as a spiral type, exhibiting a disk-like morphology, but not quite edge on. Evident spiral arm structures emanate from a central, moderately sized bulge. The arms appear flocculent, possessing a patchy and somewhat diffuse structure. Star formation appears active within these arms, as indicated by the presence of bluer regions consistent with populations of young, hot stars. The bulge is characterized by a yellowish-orange hue, suggestive of an older stellar population. There is a slight distortion on one side of the galaxy, which could be suggestive of minor gravitational interaction. The majority of the disk appears relatively undisturbed. There is a hint of a bar feature in the center of the galaxy, but it is not well defined.