The galaxy presents as a spiral type, exhibiting a relatively high degree of organization. Two distinct spiral arms are discernable, originating from a somewhat prominent central bulge. The arms appear moderately wound, neither tightly compressed nor widely dispersed. The bulge exhibits a yellowish hue, potentially indicating an older stellar population. There appears to be a slight asymmetry or disturbance in the disk and/or halo. There is no clear indication of a bar structure in the image. The disk is viewed at an oblique angle, suggesting it is not precisely edge-on but close to it.
