This galaxy presents as an edge-on spiral or lenticular galaxy, characterized by a relatively smooth and elongated morphology. A central bulge is discernible, exhibiting a reddish hue that suggests an older stellar population. Fainter, bluish light extends outwards from the bulge along the galactic plane, which is more consistent with younger stars and possibly ongoing star formation regions. This may indicate that the galaxy has some recent star formation occurring in its disk regions, although its relative paucity, along with its smooth appearance, is more consistent with a relatively quiescent galaxy. There is no indication of strong tidal features or major disturbances, although a subtle asymmetry in the disk might suggest a minor interaction or recent accretion event. 
