The galaxy presents a smooth, elliptical morphology with a high degree of central concentration. Its overall shape appears largely spheroidal, showing a subtle deviation towards a slightly elongated form. There is no discernible spiral arm structure or dust lane obscuration visible in this observation. The galaxy exhibits a color gradient, appearing more yellow-white toward its core, and becoming slightly redder in its outer regions, this suggests a population gradient of stars. No apparent tidal features or signs of recent major merger events are evident. There may be a faint disk, though it is hard to tell. There may be some minor disturbance, but it is likely not a merger.
