The galaxy presents as a flattened, disk-shaped structure, seen at a significant inclination. It exhibits a central bulge that appears relatively smooth and concentrated, with a gradual fading of light intensity from the center outwards towards the disk. The disk component shows evidence of spiral arm structures, although these are somewhat ill-defined and lack sharp contrast. There's a subtle blueness to the galaxy, particularly in the disk regions, possibly indicating recent or ongoing star formation. A noticeable dust lane is either not present, or obscured by the angle we are viewing the galaxy at. There's evidence of some minor disturbances in the disk, but it is unclear whether this is indicative of a merger or collision event. Overall, the galaxy has a smooth, ordered morphology.
