The galaxy presents a largely smooth and rounded morphology. It appears as a central, bright core surrounded by a fainter, diffuse halo of light. There is little evidence of spiral arms or a distinct disk structure. The galaxy's overall shape is generally elliptical. There might be some minor disturbances in the halo, but no obvious signs of major mergers or interactions. The color suggests a population of older stars, giving the galaxy a yellowish-orange hue, strongest in the center and diminishing outwards.
