The subject galaxy presents as an edge-on spiral, exhibiting a flattened disk morphology. Dust lane obscuration is prominent and bisects the galaxy along its major axis. The central bulge appears somewhat rounded in nature. Evidence of tidal disturbances or major merger activity is absent, although the presence of minor irregularities cannot be entirely ruled out based on this image alone. The central bulge appears brighter at bluer wavelengths while the disk is composed of redder wavelengths. The apparent dimensions of the galaxy suggest a moderate size.
