This galaxy presents as a largely featureless elliptical or lenticular structure. It exhibits a centrally concentrated luminosity profile, with brightness decreasing smoothly outwards from a bright core. There is a slight elongation, but the overall shape is generally round. I observe an even distribution of light within the galaxy. This could indicate an older stellar population with little ongoing star formation. There is no distinctive spiral arm or other similar structure detected. It is a large, high-mass galaxy at intermediate redshift. The galaxy does not appear to be undergoing any major mergers or tidal disturbances.
