The galaxy presents a generally smooth morphology, with a primarily elliptical appearance, although it does not appear to be perfectly spherical. There is a slight elongation noticeable. The galaxy exhibits a central concentration of light, with the core appearing brighter and more intensely orange-colored than the surrounding regions. The color suggests an older stellar population. The outskirts show some minor disturbances that point to a possible interaction with a different galaxy. The outer regions fade gradually into the background sky, without a well-defined edge. There appears to be some evidence of merging or tidal features surrounding the central mass of the galaxy. The image suggests a system with a high degree of spheroidal symmetry.
