The galaxy exhibits a flattened, disk-like morphology, oriented edge-on relative to our line of sight. A prominent central bulge dominates the structure, appearing smooth and concentrated with a yellowish hue, suggesting an older stellar population. The disk component is visible as a faint, diffuse band extending outwards from the bulge, with an apparent lack of distinct spiral arms. The lack of blue color within the galaxy suggests a relatively low star formation rate. Additionally, the galaxy does not display any obvious signs of a recent major merger or strong tidal disturbance, although subtle asymmetries in the disk cannot be ruled out.
