The galaxy presents as a centrally concentrated object with a smooth, diffuse light distribution. The morphology appears to be elliptical, possibly with a slight elongation. The central region exhibits a yellowish hue, suggesting an older stellar population. Moving outward, the galaxy transitions to a bluer color, indicating the presence of younger stars or a recent burst of star formation. The overall structure shows no prominent spiral arms or irregular features, further supporting its classification as an elliptical galaxy. There is no obvious dust lane or clear indication of on-going major mergers. There is a general absence of detailed structure within the galaxy.
