The galaxy appears as a flattened, disc-like structure. The central region exhibits a bright, concentrated luminosity, suggesting a prominent galactic nucleus. The light distribution becomes fainter and more diffuse towards the outer edges. There is some evidence of a subtle spiral structure or disc feature surrounding the center of the galaxy. A second object resides very close to the galaxy, which is most likely two galaxies that are in the process of a minor disturbance or merging event. There appears to be a faint stream of material connecting the two luminous objects, possibly tidal debris.
