This galaxy appears to be a relatively smooth, elliptical-type system. Its morphology is characterized by a central bulge that exhibits a bright, yellowish-white hue, suggesting a population of older stars. Moving outward from the core, the light gradually fades into a less intensely colored halo or envelope, possibly indicating the presence of a more diffuse stellar population. The galaxy’s overall shape is elongated, more like a disk than a sphere. There are only minor signs of disruption.
