The galaxy presents with a relatively compact morphology. It exhibits a disk-like structure, though features are not well-defined. There is a hint of a possible tidal interaction or minor disturbance in the morphology of the galaxy. The primary body of the galaxy shows a central concentration of light. The galaxy appears moderately bright, and displays a color gradient indicating varying stellar populations throughout. The presence of this color gradient is suggestive of differing star formation histories across the galaxy. A small fraction of the overall light output appears to be related to active star formation.
