The galaxy presents as a relatively smooth, disk-shaped structure seen nearly edge-on. There is a bright, concentrated central bulge that fades smoothly into the surrounding disk. The disk appears elongated and somewhat cigar-shaped, with a slight asymmetry in its outer regions. The color gradient suggests an older stellar population, transitioning from yellow-white in the core to redder hues further out. There is no obvious spiral arm structure or significant dust lane obscuration visible. The morphology indicates it is a galaxy with a notable bulge component and a disk, likely an early-type spiral or lenticular galaxy. No signs of active galactic nuclei or recent major merger events are immediately apparent. The smoothness and lack of pronounced features imply a relatively quiescent star formation history.
