The observed galaxy exhibits a distinct edge-on morphology. The primary structure consists of a highly flattened disk oriented perpendicular to our line of sight. A prominent central bulge is visible, exhibiting a rounded shape. The disk component displays a noticeable color gradient, transitioning from a bluer hue at the outermost edges to a redder, dustier appearance towards the midplane. Some subtle disturbances can be noted within the disk, potentially indicative of tidal interactions or internal processes. Faint hints of what could be a tidal tail can be seen extending out of the disk. There is no apparent major merger activity, although minor disturbances or interactions cannot be ruled out. 
