The galaxy exhibits a noticeable disk structure. The spiral arms are present, exhibiting a relatively open morphology. A bulge component is present, appearing somewhat compact and centrally located within the disk, but is not the dominant morphological feature. The galaxy appears to have a relatively low inclination angle to our line of sight. There is no apparent major merger activity, although subtle disturbances or irregularities in the disk's structure and arm morphology could be indicative of minor interactions. The galaxy's light profile appears smooth, and is primarily composed of intermediate to older stellar populations. There is an apparent bar structure. 
