This galaxy presents as an edge-on disk galaxy. A prominent central bulge is visible, appearing relatively large and bright. The bulge exhibits a smooth, rounded morphology. The disk itself is thin and elongated, appearing to be nearly perpendicular to our line of sight. Within the disk, some subtle color variations and slight dust lane presence is indicated, but a distinct spiral structure is not readily apparent due to the edge-on perspective. The galaxy's overall color suggests a mixture of stellar populations, with the bulge potentially being populated by older, redder stars, while the disk may contain younger, bluer stars. The galaxy exhibits a small disturbance. There is no indication of a recent or ongoing major merger.
