The observed galaxy presents as an edge-on spiral with a clearly defined disk. Dust lanes appear to be present. The central bulge is moderately prominent and appears somewhat elongated, with a color suggesting an older stellar population. Faint, blue-tinged spiral arms are discernible extending from the central bulge, indicating areas of ongoing star formation. There is some indication of asymmetry within the disk, which could be caused by minor gravitational interactions or internal disturbances. No major mergers are evident. The general morphology points to a significant disk component. The spiral structure is faint but extended.
