The galaxy presents as a flattened, elliptical structure, viewed nearly edge-on. A bright, concentrated central bulge is visible, displaying a yellowish hue, which may indicate an older stellar population and reduced star formation in that region. The disk component is characterized by a more diffuse, bluish color, suggesting the presence of younger, hotter stars and ongoing star formation. Some irregularities and a slight warp are observable in the disk, potentially due to minor gravitational interactions or internal dynamic processes. A hint of dust lanes appears to be present along the plane of the disk, obscuring some of the light from the bulge. There are no obvious signs of a major merger, though a minor disturbance cannot be ruled out based on the morphology.
