The galaxy presents a relatively smooth, elliptical morphology. It exhibits a centrally concentrated luminosity profile, with the brightest region appearing almost stellar-like. The light gradually decreases in intensity toward the outer regions of the galaxy. There is a distinct lack of spiral arm structure or prominent dust lanes. Color gradients are present; the central region is a mix of colors which fade slightly to the outer regions of the galaxy. Some minor disturbances appear to affect the galaxy's morphology. This suggests a past or ongoing interaction, although no major merger events are currently visible. The overall appearance is consistent with an evolved stellar population and suppressed star formation.
