The galaxy appears to be a spiral type, exhibiting well-defined spiral arms. These arms are traced by regions of active star formation, indicated by their bluer color. The central bulge is not particularly dominant, appearing moderately sized relative to the disk. There isn't strong evidence of a bar structure. The galaxy's disk is not viewed edge-on, presenting a more face-on orientation. Overall, the galaxy exhibits signs of ongoing star formation and a relatively undisturbed morphology. There are no signs of a major merger event occurring; however there may be minor disturbances present.