The galaxy appears as a smooth, elliptical-shaped object, exhibiting a high degree of central concentration. Its color profile indicates an older stellar population, leaning towards redder wavelengths. There is a very subtle indication of a minor disturbance in its morphology, such as a slight asymmetry or faint tidal feature, suggesting the possibility of a past or ongoing interaction with a smaller galaxy or object. The galaxy's lack of prominent spiral arms or dust lanes further supports its classification as an elliptical. Its small angular size suggests that it is a galaxy that is at a significant distance. Based on the light we see, this system has a low star-formation rate and exhibits a significant mass. 
