The galaxy presents as a somewhat elongated structure, exhibiting a smooth, centrally concentrated light profile. The core region appears brighter and exhibits a yellowish hue, which may indicate an older stellar population with minimal ongoing star formation. The outer regions show a slight flattening and a decrease in luminosity as you move away from the center, with a faint extension along its major axis. There are some very subtle hints of possible minor disturbances in its structure, suggesting a potential interaction or past merger event. The overall morphology suggests a possible classification as an elliptical or lenticular galaxy.
