The galaxy presents as a highly inclined, possibly edge-on, disk galaxy. A prominent central bulge dominates the galaxy's morphology, exhibiting a smooth, concentrated light profile with a yellowish hue. The disk component is faint and elongated, appearing relatively featureless without distinct spiral arm structures visible at this resolution. The colors suggest that the bulge may contain older stellar populations. No significant tidal features or obvious signs of a major ongoing merger are apparent. However, minor disturbances within the disk cannot be ruled out with certainty given the image quality.
