The galaxy presents as a disk-shaped system, viewed nearly edge-on from our line of sight. The central region exhibits a strong concentration of light, appearing yellowish-white, suggestive of an older stellar population. The outer disk appears flattened with no distinct spiral arm structure visible. The dust lane is prominent, obscuring a significant portion of the mid-plane region, creating a contrast between the brighter central bulge and the fainter outer disk. There appear to be no signs of any major mergers or tidal disturbances present. There is a strong suggestion of disk morphology with a round bulge.
