The galaxy presents as a spiral type, exhibiting a well-defined disk structure. Prominent spiral arms are visible, extending outwards from the central region. The arms appear somewhat flocculent in nature. There appears to be moderate levels of dust obscuring the disk and spiral arm structure.

The central bulge of the galaxy appears relatively small or non-existent. There is no clear evidence of a strong central concentration of light. There also appears to be possible signs of minor interaction or disturbance. There are some asymmetries visible in the outer regions of the spiral arms, indicating potential gravitational influence from a nearby object.
