The galaxy presents as an edge-on spiral. It appears highly elongated, with a notably high axial ratio indicating a significant inclination relative to our line of sight. A prominent central bulge is observed, displaying a smooth, concentrated luminosity profile. Faint dusty features are visible throughout the disk. The integrated color suggests an evolved stellar population, with a redder hue implying a lower specific star formation rate. There's a hint of slight asymmetry in the disk's morphology, potentially indicating minor gravitational interactions or recent accretion events. The absence of well-defined spiral arm structures suggests either a smooth stellar distribution in the disk or obscuration by dust lanes.
