The galaxy presents as a moderately bright, elliptical-shaped object with a smooth light distribution. Its core region exhibits a concentrated, luminous glow, transitioning gradually into a fainter, more diffuse halo. The color gradient suggests a population of older stars, with a central bulge appearing more yellow/orange. There are no distinct spiral arms or prominent dust lanes visible, which further supports its classification as an elliptical galaxy. A slight elongation is observed, suggesting a deviation from a perfectly spherical shape. There are no visible signs of ongoing major mergers, though subtle irregularities in the outer regions cannot be ruled out based solely on this image.
