The galaxy presents as a single, somewhat amorphous object with a generally elliptical shape, but there are no spiral arms or a well-defined disk structure readily apparent. The light appears to be concentrated toward the center, indicating a bulge or a core region. This central area is visibly brighter than the outer regions, implying a higher density of stars. The outer regions gradually fade into the background, suggesting a decreasing stellar density with increasing radius. The overall color appears to be on the redder end, indicative of an older stellar population and limited active star formation. There are some minor asymmetries or disturbances visible in the outer regions, hinting at a possible past interaction or merger event.
