The galaxy appears to be a spiral galaxy, exhibiting a notable disk structure. The arms are tightly wound around a central bulge. The bulge appears moderate in size relative to the overall disk. There are indications of active star formation within the spiral arms, as evidenced by the bluer hues present. The galaxy does not show signs of any major interactions or mergers and appears relatively undisturbed. The galaxy disk is not perfectly edge-on and is instead seen at an angle relative to our line of sight.
