This galaxy exhibits an elliptical morphology, appearing generally smooth in texture with a central bulge that dominates its luminosity profile. The color index suggests an older stellar population, possibly with ongoing or recent star formation. There is a hint of asymmetrical features, which could be evidence of a minor disturbance or interaction. The galaxy appears to be experiencing a merger. There is a slightly elongated shape to the galaxy. There are a few bright regions which likely correlate with star formation.
