The galaxy presents as a disk galaxy, oriented approximately face-on relative to our line of sight. The central bulge appears prominent, exhibiting a bright, concentrated luminosity. Spiral arm structures are present but somewhat indistinct, appearing flocculent rather than grand design. The arms are visible as subtle variations in color and density extending outwards from the central bulge.

There is an asymmetry to the overall light distribution within the galaxy. One side of the disk is slightly more extended or brighter than the other. No tidal features or obvious signs of interaction are observed. The color suggests an intermediate redshift, as the blue is attenuated. There is a hint of dust lanes obscuring some light in the arms. The light of the central bulge, particularly the core, is comparatively very bright.
