The galaxy presents as a relatively faint, elongated structure. Its core exhibits a yellowish hue, suggesting an older stellar population or dust obscuration. Surrounding the central bulge is a diffuse disk, appearing bluish, indicative of younger stars. The morphology suggests an edge-on spiral or lenticular galaxy. There is a very slight hint of asymmetry in the disk, potentially indicating a minor disturbance or interaction. The galaxy appears relatively smooth, with no clear signs of spiral arms. The overall shape is markedly elongated, with a cigar-like form.
