This galaxy appears to be a spiral galaxy viewed edge-on. A prominent bulge is visible, exhibiting a yellowish hue suggesting an older stellar population. The disk presents a flattened structure with a faint bluish tint, potentially indicative of younger stars and ongoing star formation. The disk appears relatively smooth, lacking large distinct spiral arm structures. There is a subtle warping or flaring visible at the outer edges of the disk. There is no obvious evidence of a major merger event, though minor disturbances cannot be ruled out. Overall, the galaxy appears to be a relatively massive system with a moderate rate of star formation.
