The galaxy presents as a relatively smooth structure, although subtle features are apparent. It appears to be an elliptical or lenticular type galaxy, exhibiting a flattened shape. The central region displays a higher concentration of light, suggesting the presence of a bulge. The light distribution transitions gradually outwards from the center to the outer edges. The color profile is relatively consistent across the galaxy, trending towards the red end of the spectrum, indicating an older stellar population. Irregularities are visible, suggesting a possible ongoing merger with another galactic structure, or the remnant of a past interaction. There are also visible arms of gas and dust around the outside of the center of the galaxy.