The galaxy presents a predominantly disk-like morphology, exhibiting discernible spiral arm structures. These arms appear tightly wound around a central bulge, with a moderate contribution of the bulge relative to the overall disk size. The winding tightness suggests a classification towards the later end of the spiral sequence, likely Sa or Sb.

The galaxy displays a slight ellipticity. The light distribution indicates a centrally concentrated profile with a decreasing intensity towards the outer regions of the disk. A bar may be present but this cannot be confirmed, the galaxy shows a smooth overall appearance with some features present in the spiral arms. There does not appear to be evidence of any major merging or disturbances and it appears as a relatively isolated galaxy.
