The galaxy appears to be a spiral galaxy, viewed at a high inclination, nearly edge-on. The central bulge appears prominent and elongated, exhibiting a yellowish-orange hue, suggestive of an older stellar population. Fainter, bluish light can be seen in one of the edges of the disk, which may indicate regions of more recent star formation. The dust lane is not clearly visible but there are hints of it within the disk. The disk itself is moderately extended, with a smoother appearance. Some faint signs of disturbance, such as minor asymmetry, may be present in the outer regions of the disk.
