The galaxy displays a distinct spiral structure, characterized by two prominent arms extending from a central bulge. These arms appear loosely wound and extend outwards, suggesting an Sb or Sc classification on the Hubble sequence. The central bulge is relatively small compared to the overall disk size. A bar-like structure is visually apparent, bisecting the bulge and extending into the inner regions of the spiral arms. The disk shows a blue hue, indicative of ongoing star formation within the spiral arms. Areas of increased brightness are present within the arms which likely correspond to regions of active star formation. There is a noticeable asymmetry to the spiral arm structure, with one arm appearing more extended and diffuse. Some level of gravitational disturbance is observed.
