The observed galaxy appears to be a spiral galaxy, exhibiting a well-defined disk structure. The spiral arms are prominent, displaying a moderate winding pattern, though the low resolution of the image limits detailed tracing. The arms appear symmetrical, with at least two clearly visible.

A central bulge is present, though not especially dominant, and the disk shows some evidence of a bar feature traversing the center of the bulge. The galaxy is neither viewed edge-on nor face-on, but at a moderate inclination allowing the spiral structure to be observed. There is no obvious sign of active merging or major tidal disturbances, though minor asymmetries could indicate past interactions. The galaxy exhibits a blue hue, which may indicate active star formation.
