The galaxy appears to be an elliptical galaxy, exhibiting a smooth, diffuse morphology. The light profile suggests a centrally concentrated bulge. There appears to be minimal evidence of spiral arms or significant dust lanes. The galaxy possesses a reddish-yellow hue, suggesting an older stellar population with relatively low current star formation. There are no obvious signs of a major ongoing merger, though minor disturbances cannot be ruled out at this resolution. It has a shape that is between round and elongated.
