This galaxy presents as a flattened, elongated structure, consistent with an edge-on or highly inclined disk galaxy. The central bulge is prominent, exhibiting a yellowish hue that may indicate an older stellar population and potentially a higher concentration of dust. Moving outward from the bulge, the disk becomes bluer in color. This color transition suggests younger, hotter stars may dominate in the outer regions of the disk, perhaps indicating ongoing star formation. Overall, the galaxy displays a smooth texture, although subtle features like dust lanes might be present, given the edge-on viewing angle. The general morphology indicates a well-formed, potentially undisturbed system that is undergoing stellar evolution.
