This galaxy presents a striking edge-on disk morphology. A prominent central bulge is observed, characterized by a smooth, rounded profile and a relatively concentrated light distribution. The disk appears thin and elongated, obscuring the galactic nucleus with dust. Light emanating from the galaxy is primarily in the redder portions of the spectrum, suggestive of an older stellar population or significant dust obscuration. There is no obvious sign of active galactic nuclei or merging activity. Star formation appears to be low. 
