The galaxy presents as a spiral type, with a significant disk component viewed at a non-edge-on angle. The presence of spiral arms is apparent. A central bulge is noticeable, appearing to be a moderate size relative to the disk. There's evidence of a bar-like structure traversing the central region of the galaxy. The galaxy's light distribution appears relatively smooth, with a centrally concentrated luminosity profile. Color gradients suggest some degree of ongoing star formation, particularly in the disk regions. The galaxy shows no obvious signs of a major merger event, but there may be some minor disturbances in its morphology. Overall, the galaxy appears to be a relatively normal spiral galaxy at a redshift of approximately 0.083.
