The galaxy presents as a smooth, elliptical-like structure. Its overall shape is somewhat elongated, but with a noticeable concentration of light towards the center. There appears to be a gradual decrease in luminosity from the core outwards, lacking distinct spiral arms or irregular features. A subtle color gradient is present. The central region exhibits a slightly yellowish-white hue, which fades to a bluer tint in the outer regions. Based on the apparent lack of defined features, and color gradient, star formation may be present, but is concentrated in the outer regions. The galaxy exhibits a minor disturbance or some type of ongoing interaction that slightly perturbs the overall shape, but does not appear to be undergoing a major merger.
