The galaxy presents as a moderately luminous object with an apparent elliptical morphology. The central region appears relatively smooth and concentrated. The light profile suggests a single, dominant spheroid component, with a noticeable lack of spiral arm structures or distinct features that would indicate active star formation in a disk. There is a slight color gradient, transitioning from a more yellow-orange hue in the center to a bluer tint toward the outer regions, which may suggest a radial change in stellar populations. A visual inspection of the galaxy's shape suggests it appears moderately rounded. The overall appearance hints at a galaxy that may be in the later stages of its evolution, possibly transitioning toward a more quiescent state. Evidence suggests a moderate possibility of merger activity, but the degree of disturbance is minor, if present. 
