The galaxy presents as a spiral, with a defined disk structure. Two prominent spiral arms extend from the central region. These arms appear relatively well-defined, exhibiting a medium winding, suggesting an intermediate spiral type.

There is a slight suggestion of a bar-like feature spanning the galaxy's core, but it is difficult to discern it from this angle. The bulge appears moderate in size relative to the disk. The galaxy's inclination is such that the disk is viewed nearly face-on.

The color distribution across the galaxy suggests regions of active star formation within the spiral arms.

The overall morphology points to a galaxy undergoing relatively normal spiral structure evolution, though some minor disturbances are apparent within the disk, perhaps the result of small gravitational interaction.
