The observed galaxy presents a distinctly edge-on disk morphology. It exhibits a prominent central bulge which appears to be generally rounded. The disk is relatively thin and elongated, extending significantly beyond the bulge. There are faint indications of possible minor disturbances or irregularities within the disk structure, but it is largely undisturbed. No strong signs of ongoing or recent major merger events are apparent. Overall, the galaxy appears relatively smooth in its overall light distribution, with some internal features discernible.
