The galaxy presents an apparent disk-like morphology, oriented at an oblique angle relative to the line of sight. There appears to be a bright, concentrated central bulge with a somewhat defined edge, suggesting the presence of a supermassive black hole. The disk shows some color variation from the central region outward with a change in the intensity. The presence of a possible disturbance in the disk region of the galaxy suggests a potential recent minor merger or tidal interaction. There is an artifact near the galaxy that distorts the shape of the light.
