The galaxy presents as an edge-on spiral, displaying a flattened disk shape. The central bulge appears prominent and smoothly luminous, exhibiting a slight yellowish hue, possibly indicative of an older stellar population. The disk itself shows a gradient in color, with a transition from the yellowish central region to a bluer tint towards the outer edges. This suggests ongoing star formation within the disk. No strong dust lanes are immediately apparent. There are no signs of any major merger events, but there are minor disturbances. It exhibits a relatively smooth profile. 
