The galaxy presents a largely smooth, elliptical morphology. The core exhibits a bright, concentrated luminosity, gradually decreasing in intensity towards the outer regions. It appears to have a nearly circular shape, with no significant asymmetries or tidal features visibly apparent. The color gradient suggests a stellar population that is primarily evolved, with a dominant yellowish-red hue in the central region and a slightly bluer tint in the outer portions of the galaxy. There is no evidence of ongoing or recent major merger activity or significant dust lanes. The galaxy appears relatively undisturbed, consistent with a relaxed stellar system.
