The galaxy presents a largely smooth, elliptical morphology. Its light profile exhibits a strong central concentration, with a gradual decrease in luminosity outwards. The galaxy appears mostly featureless in the available imagery, without evidence of spiral arms or a distinct disk structure. It exhibits a roughly round shape. There is no strong visual evidence of ongoing major mergers or tidal disturbances in this image, though minor interactions cannot be fully ruled out. The color profile suggests a population of older stars, giving it a yellowish-red hue, potentially indicating relatively low current star formation activity.
