The galaxy appears as a slightly elongated, luminous object. It is relatively smooth in appearance, lacking any prominent spiral arms or bar structures. The light distribution suggests a centrally concentrated bulge, with a gradual decrease in luminosity towards the outer regions. The color is subtly reddish, which could indicate an older stellar population or dust obscuration. There are no obvious signs of active galactic nuclei activity or recent major mergers. There is a slight asymmetry. Overall, the galaxy presents itself as a relatively quiescent system, likely an elliptical or lenticular galaxy seen at a moderate distance.
