The galaxy presents as a relatively faint, disk-shaped object, observed edge-on. It exhibits a slight reddish hue, suggesting older stellar populations or significant dust obscuration. The galaxy has a moderately luminous bulge, somewhat rounded in appearance, lacking obvious features like boxiness. The disk appears relatively smooth, without distinct spiral arm structures or prominent star-forming regions visible at this resolution. There is no clear evidence of a major ongoing merger or significant tidal disturbances affecting the morphology. The disk extends to a considerable length. The overall shape is consistent with a late-type spiral galaxy or a lenticular galaxy viewed edge-on.
