The galaxy presents an elliptical morphology, exhibiting a smooth and concentrated light distribution, with a high degree of roundness. There is a relatively homogeneous color gradient across the entirety of the galaxy. There is no strong evidence of spiral arm structures, dust lanes, or significant star forming regions visible in this image. The galaxy exhibits a smooth appearance with no apparent major disturbances indicating recent or ongoing major merger events. The galaxy has an estimated radius of approximately 7 kpc. The overall color suggests a relatively mature stellar population.
