The galaxy presents a morphology indicative of a spiral galaxy, viewed at an oblique angle. Its disk exhibits a dominant presence, characterized by a prominent central bulge. Traces of spiral arm structure are visible, though somewhat ill-defined. These arms appear to be loosely wound. There appears to be a faint possible merger or tidal disturbance at the top of the galaxy, the tidal features are not as pronounced. The lack of a clear dust lane and the brightness of the galaxy suggest minimal dust extinction along the line of sight.
