The galaxy presents a generally smooth and centrally concentrated light distribution, with an apparent elliptical morphology. There is a slight elongation, with an axis ratio indicating a departure from a perfectly circular shape. The galaxy exhibits a color gradient, with the central region appearing more yellow-red, potentially indicating an older stellar population or higher dust extinction. The outer regions show bluer colors, suggesting the presence of some younger stars, but overall the blue component is subdued. No prominent spiral arms or distinct features such as star-forming regions are discernible within this image. There may be slight disturbance on the edges, but otherwise appears relatively undisturbed.
