The galaxy presents as an elongated, disk-shaped structure, likely an edge-on spiral or lenticular galaxy. A central bulge is clearly visible, exhibiting a yellowish-white color, which may indicate an older stellar population. The disk surrounding the bulge appears relatively smooth. There is minimal evidence of spiral arm structure. The galaxy's overall color suggests a more evolved system, possibly with ongoing star formation. There is no visually obvious sign of strong gravitational interaction or major merging activity; there may be minor disturbances in the disk. Dust lanes are not readily apparent, although the dark regions on either side of the bulge suggest some obscuration.
