The galaxy appears to be an elliptical galaxy. The light distribution is generally smooth and centrally concentrated, lacking prominent spiral arms or a well-defined disk structure. The overall shape is quite round, though it could possibly be described as in-between round and elliptical. There appears to be an intense region in the center. There appears to be a secondary point of light to the right of the central area. There does not seem to be a large amount of active star formation present. The galaxy appears to be a large, relatively evolved system. There is evidence of tidal interactions or a possible merger in progress, as evidenced by a plume-like or distorted shape that surrounds the galaxy's primary body.
