The galaxy presents a discernible spiral structure. Two prominent arms emanate from a central bulge region, exhibiting a medium winding pattern. The bulge appears to be of moderate size.

The spiral arms are well-defined and show some patchiness, potentially indicating regions of active star formation. There is an indication of two dominant spiral arms. The galaxy is oriented face-on with respect to our line of sight, allowing a clear view of its spiral structure.

There is a suggestion of a bar-like structure across the center of the galaxy. Based on visual inspection, the degree of disturbance is considered none, and there is no indication of merging activity.
