The galaxy presents as a spiral galaxy with a relatively high degree of disk inclination. A well-defined central bulge is present. Faint spiral arm structures appear to emanate from the central region. These arms are somewhat flocculent in nature, displaying a patchy distribution of star formation.

There is no evidence of a strong bar structure crossing the bulge, but there may be a weak bar. The outer regions of the disk exhibit a bluer color, indicative of ongoing star formation activity. The galaxy does not show obvious signs of major interaction or merging, although some minor disturbances cannot be ruled out. Overall, the galaxy exhibits a complex morphology indicative of ongoing evolutionary processes.
