The galaxy presents a smooth, elliptical morphology. It exhibits a concentrated central region with a relatively gradual decrease in luminosity towards its outer edges. The color profile suggests a population of older stars, with a yellow-orange hue dominating the central region. There is a faint hint of bluer light in a less-defined area, indicating a small amount of ongoing star formation. The overall structure indicates that it is most likely an older galaxy that may have undergone some minor interaction events. There is no distinctive spiral arm structure or a defined disk, the object being predominantly spheroidal in shape.
