The galaxy presents as an edge-on or nearly edge-on disk galaxy. A central bulge is visible, appearing bright and concentrated. The disk component is elongated and exhibits a relatively smooth texture, although some faint, subtle structural features may exist within. The galaxy appears more luminous in the redder wavelengths and less luminous in the bluer wavelengths. Overall, there are no major indications of tidal disturbances or ongoing merger activity, such as tails, lopsidedness, or strong asymmetries in the disk.
