The galaxy presents as an edge-on spiral, characterized by a prominent, elongated disk. The central bulge appears substantial and exhibits a rounded morphology, with a concentration of older stellar populations inferred from its yellowish-orange color. The disk component shows a dust lane bisecting the galaxy, obscuring some of the light from the bulge. Star formation appears to be suppressed throughout the galaxy. No significant tidal features or distortions indicative of recent major merger activity are discernible. There is no bar-like structure.