The galaxy presents a generally smooth, rounded morphology. Its central region exhibits a bright, concentrated core, suggesting a significant stellar density. The overall color appears to be on the redder end of the spectrum, possibly indicating an older stellar population or significant dust obscuration. There is a slight elongation, but overall the galaxy appears relatively undisturbed with the appearance of a minor disturbance. Based on its high mass, it is likely a large and evolved system. Based on the low levels of recent star formation it is likely an elliptical galaxy.
