The galaxy appears to be relatively compact and disk-like, viewed nearly edge-on. There is a distinct central bulge that is fairly prominent. The galaxy exhibits a blue-green coloration, which could indicate active star formation within the disk. Faint extensions or tidal features may be present perpendicular to the main disk plane, suggesting potential gravitational interactions or past merger events, though any strong signs of interaction or a disrupted morphology are not obvious at first glance. There is a narrow dust lane seen obscuring the central bulge along the plane of the galaxy. The disk shows a smooth light distribution without clear spiral arm structure.
