The galaxy presents as an elongated, disk-like structure viewed nearly edge-on. There is a noticeable central bulge, appearing brighter and slightly yellowish, suggesting an older stellar population concentrated towards the galaxy's center. The disk exhibits a bluer hue, particularly towards the outer edges, possibly indicating ongoing star formation within spiral arms or a younger stellar population. Dust lanes appear to be present, obscuring some of the starlight along the central plane of the galaxy. The overall morphology is consistent with a spiral or lenticular galaxy seen at a high inclination. There are no obvious signs of major tidal disturbances or recent merger events.
