The galaxy presents a relatively smooth, elliptical morphology. Its core exhibits a high degree of luminosity and concentration, indicating a substantial stellar population within that region. The galaxy displays a gradual decrease in brightness from the central region outwards, with no apparent distinct spiral arms or features. There is a slight elongation in its shape. The galaxy's color suggests a population of older stars, with a redder overall hue as opposed to the bluer colors associated with active star formation.
