The galaxy presents as a relatively faint, edge-on spiral system. A distinct bulge region is visible, elongated along the major axis. The disk appears diffuse, with limited resolution preventing a detailed assessment of spiral arm structure. The system exhibits a noticeable color gradient, transitioning from a bluer hue at the outer edges of the disk, possibly indicating areas of recent or ongoing star formation, to a more yellowish and red central bulge, which could represent an older stellar population. There is a slight warping of the disk. There is some potential indication of minor disturbance. 
