The galaxy presents as a fairly smooth, centrally concentrated object. The light distribution suggests a dominant spheroid component. There is a slight flattening or disk-like feature. There are some faint outer structures, but these do not indicate a strong ongoing merger event. The galaxy exhibits a color gradient, appearing more yellow or golden in its core region, transitioning to bluer hues in the outer regions, possibly indicating regions of more recent star formation. Overall, the morphology suggests an intermediate type, likely between a lenticular and a spiral galaxy with tightly wound arms.
