The galaxy presents as a spiral structure, viewed at an angle oblique to face-on. The spiral arms are clearly defined. They exhibit a tightly wound morphology, with evidence of ongoing star formation indicated by their bluer colour. The central bulge is comparatively small. There appears to be a bar feature crossing the central region of the galaxy. The overall form suggests a classification of a barred spiral galaxy, exhibiting a prominent disk component with a notable presence of spiral arms. There is a hint of interaction or minor disturbance in the galaxy's morphology, which would have to be substantiated with additional data.
