The observed galaxy appears as an edge-on spiral or lenticular galaxy. A prominent central bulge dominates the visual structure, exhibiting a smooth, concentrated morphology with a yellowish hue, suggesting an older stellar population within. A faint disk extends outward from the bulge. The disk appears thin and elongated, with hints of a more bluish color indicative of younger stars. The lack of distinct spiral arm structures indicates a relatively smooth stellar distribution. The galaxy does not appear to be undergoing any major merger events, though minor asymmetry within the disk cannot be ruled out.
