The galaxy presents a distinctly elongated, cigar-like morphology. Its light profile appears relatively smooth, lacking any prominent spiral arm structures or distinct features typically associated with grand design spirals. The central region exhibits a concentration of light, suggesting a potential bulge component. The galaxy's color gradient shows a transition from a yellowish core to slightly bluer hues at its edges, possibly indicating the presence of younger stellar populations in the outer regions. The overall shape suggests it may be an elliptical galaxy seen edge-on, or a lenticular galaxy with a prominent disk. There is no obvious dust lane. There is no clear evidence of a major ongoing merger, however there could be a recent minor disturbance based on the smoothness.