The galaxy presents as an edge-on spiral with a prominent central bulge. The bulge exhibits a smooth, rounded morphology. A disk extends outwards from the bulge, appearing relatively thin and elongated, with evidence of moderate star formation occurring. There is no readily apparent strong disruption or tidal features indicating any recent major mergers. The overall structure suggests a relatively undisturbed evolutionary state. The galaxy is moderately luminous, with a stellar mass that is fairly high.
