This galaxy appears to be a spiral galaxy, oriented edge-on relative to our line of sight. A prominent central bulge is observed, appearing luminous and relatively smooth. The bulge transitions into a fainter, extended disk, which is significantly flattened and displays a dust lane. The disk exhibits some irregularity, suggesting possible gravitational interactions or recent merger activity. The color gradient from the bulge to the disk suggests a possible change in stellar populations, with older stars dominating the bulge. The galaxy appears moderately redshifted.
