The galaxy presents as a luminous, elliptical object. It exhibits a smooth, largely featureless morphology with a moderate concentration of light towards the center. There appears to be a gradual decrease in luminosity from the central core outward, with a slightly elongated shape along one axis, resembling a cigar shape. The color profile indicates a population of older stars, with a yellowish-red hue dominating. The overall structure suggests a system that is dynamically relaxed, possibly in the later stages of its evolution with minimal signs of ongoing major mergers or significant star formation. There are hints of minor disturbances, but they are not distinctly visible.
