The galaxy presents as a spiral type, observed at an oblique angle. It possesses discernible spiral arm structures that emanate from a central bulge. The bulge appears relatively modest in size. Evidence for a bar structure is suggested. The galaxy's disk is apparent, with some features potentially disrupted. No obvious signs of major mergers are evident, although subtle disturbances may be present. The overall morphology is predominantly disk-like, but some portion of the galaxy appears smooth. There are indications of on-going star formation.
