The galaxy presents as a slightly inclined disk galaxy, seen at an angle between face-on and edge-on. There's a central bulge region of increased brightness, appearing somewhat amorphous rather than a distinctly defined structure. The disk shows hints of spiral arm structure, but they are poorly defined and appear flocculent, with a clumpy distribution of brighter regions indicative of star-forming regions within the disk. The dust lanes are not easily discernible, but there is evidence of patchy extinction. The overall color of the galaxy suggests a mix of stellar populations. There is no sign of a significant bar structure. The general morphology points toward a later-type spiral galaxy.