The galaxy presents as a spiral galaxy with a discernible disk. The spiral arms are prominent, showing a mix of winding tightness, with some areas appearing more tightly wound than others. A dominant two-arm spiral structure is visible.

There is a suggestion of a bar feature crossing the central bulge, with what appears to be a strong component to its structure. The bulge itself appears small relative to the disk, showing indications of a weak dominance of the bar feature.

The overall appearance suggests some degree of disturbance or interaction, possibly a minor merging event. The morphology appears asymmetrical, showing evidence of tidal interactions, with distorted spiral arm features. 

There are regions of notable star formation within the spiral arms.

The galaxy is seen at a slight inclination.
