The galaxy presents as an elongated, disk-like structure with a prominent central bulge. The bulge exhibits a yellowish hue, suggesting an older stellar population, while the disk shows hints of bluer regions, possibly indicating ongoing star formation. The galaxy's profile appears relatively smooth, with some indications of minor disturbances or irregularities in the outer regions of the disk. The orientation is close to edge-on, obscuring detailed spiral arm structures, if any exist. There seems to be little if any dust. Overall, the galaxy appears to be a relatively evolved system.
