The galaxy presents as a relatively smooth and centrally concentrated object. The light distribution suggests an elliptical morphology or a disk galaxy seen face-on with minimal visible spiral structure. The color appears to be a yellowish hue, potentially indicative of an older stellar population with a lower rate of current star formation. The overall appearance is that of a galaxy that may have undergone significant evolutionary processes, possibly transitioning towards a more quiescent state. There are some signs of minor disturbances around the galaxy, suggesting possible past minor mergers. It appears neither highly distorted nor undergoing a major merging event at present. The shape is relatively circular.
