The galaxy presents as a relatively compact, edge-on disk galaxy. There appears to be a central bulge, significantly brighter and more concentrated than the surrounding disk. The bulge exhibits a smooth texture, with no apparent substructure. The disk of the galaxy is noticeably thin and elongated, viewed nearly edge-on. Within the disk, there's some evidence of dust lanes or obscuring material, primarily visible as darker regions silhouetted against the brighter disk. The disk shows faint hints of spiral structure or other irregularities. Diffuse light extends beyond the main disk, possibly a faint halo or tidal streams, but the signal is weak. Overall, the galaxy appears to be relatively quiescent, with no obvious signs of major star formation activity or strong tidal interactions. The color profile suggests a population of older stars within the bulge, while the disk may contain a mix of younger and older stellar populations.
