The galaxy presents a generally smooth, elliptical morphology. Its light is concentrated toward the center, indicating a prominent bulge. The color profile suggests a population dominated by older stars, particularly within the central region, which exhibits a yellow-orange hue. Moving outward from the core, the galaxy displays a gradual decrease in brightness, lacking any sharp edges or defined spiral arm structures. A subtle disk-like structure may be present, but is not prominent. There is no visible evidence of active star formation regions within this galaxy. Furthermore, the overall shape and lack of significant asymmetry suggest that this system has likely undergone significant dynamical relaxation and is not currently experiencing any major merging events. Any merging going on now would be minor. Overall, the galaxy appears to be a massive, evolved system, exhibiting characteristics consistent with an elliptical galaxy at a moderate redshift.
