The galaxy presents as a spiral, exhibiting a disk-like morphology. There are indications of ongoing or past interactions, supported by the disturbed spiral arm structure, with signs of significant tidal distortions.

The galaxy hosts a prominent bar feature bisecting the central region. There appears to be a central bulge, with the prominence of the bulge categorized as moderate relative to the overall size of the galaxy. The spiral arms display a winding pattern that appears mostly medium in tightness. 

Color gradients within the disk suggest variations in stellar populations. There appear to be two dominant spiral arms, but many cannot be classified due to the disturbance. The overall color of the disk implies substantial star formation activity with a blue tinge dominating.

Indications of tidal features and morphology suggest some sort of a merger event, with strong tidal distortions. The mass is average, suggesting this may be a common garden variety type of spiral galaxy.