The galaxy exhibits a discernible disk structure, though not perfectly face-on, presenting a slightly inclined view. Within the disk, evidence of spiral arm structures is apparent. These arms appear somewhat loosely wound and flocculent. There is a central bulge component that does not appear highly dominant in size compared to the disk. The galaxy's color profile indicates ongoing star formation, as suggested by bluer hues within the spiral arms. Indications from the image point towards potential interactions or disturbances, with some irregularities in the disk's overall morphology. Furthermore, signs of a bar are present, though not a strong one.
