This galaxy appears to be a lenticular or early-type spiral galaxy, viewed edge-on or at a high inclination angle. The central bulge is prominent and exhibits a smooth, concentrated light profile, suggesting an older stellar population. Surrounding the bulge, there is evidence of a faint, flattened disk. The disk shows a bluer color than the bulge. There may be evidence of low-level star formation within the disk, consistent with the blue color. Overall, the galaxy does not show signs of significant recent merger activity or major disturbances, maintaining a relatively regular and undisturbed morphology. The shape is elongated with a high ellipticity. 
