The galaxy presents as an elongated, edge-on disk galaxy. The central bulge appears prominent and exhibits a yellowish-orange hue, suggesting an older stellar population. The disk structure is clearly visible, extending from the central bulge. The disk shows a slight colour gradient, with the regions closer to the bulge exhibiting a similar yellowish-orange hue, and the outer regions transitioning towards a bluer tone. This potentially indicates ongoing star formation within the disk, with a higher concentration of younger, bluer stars in the outer regions. There does not seem to be evidence of a significant dust lane. The overall structure appears relatively undisturbed, without major asymmetries or tidal features indicative of recent major merger events. There might be some minor disturbances. The bulge seems smooth. The shape of the bulge seems rounded.
