The galaxy presents as a spiral galaxy, exhibiting a disk-like structure. Prominent spiral arms are observed extending outward from a central bulge. The spiral arms are not tightly wound, suggesting a later Hubble type. The central bulge appears moderately sized in comparison to the overall disk. Evidence suggests the presence of a bar structure, although it is not distinctly strong. There may be a small amount of merging, or some other sort of disturbance. Star formation appears to be relatively low. The galaxy is not seen edge-on.
