The galaxy presents a largely smooth, elliptical morphology. It exhibits a dominant central bulge with a diffuse, extended halo. There is a slight asymmetry and a hint of a possible disk component, or perhaps tidal disturbance, evidenced by faint, elongated features extending from one side of the galaxy. Color gradients suggest an older stellar population dominating the bulge, with hints of ongoing or recent star formation in the outer regions due to some bluer regions. Based on the smooth central mass distribution, a supermassive black hole is likely present at the galaxy's core. Overall, the galaxy appears to be in a relatively relaxed state, with no major ongoing merger events or intense starburst activity clearly visible.
