The galaxy presents a smooth, elongated morphology, suggestive of an elliptical or lenticular type. It exhibits a concentrated central bulge that is bright and appears nearly white. The galaxy gradually fades outwards from this central region, transitioning to a less defined outer halo.

A disk is likely present, but it is seen nearly edge-on, giving the galaxy its cigar-like shape. There are no prominent spiral arms or distinct features visible in the disk. The lack of strong color variation within the galaxy, along with the smooth appearance, suggest that star formation rates may be relatively low. There is no apparent major disturbance of its shape nor is there an indication of any ongoing merging events. 
