The galaxy presents as a spiral, exhibiting a distinct disk structure. Two major spiral arms appear to emanate from a relatively bright, compact central bulge region. These arms display a somewhat flocculent structure, with apparent breaks and segments rather than continuous, well-defined patterns.

The galaxy appears relatively face-on. There's evidence of ongoing star formation within the spiral arms, indicated by the presence of bluer regions and patches associated with younger stellar populations. Indications of disturbances are present in the outer arms.
