The galaxy presents a largely smooth, elliptical morphology, appearing well-rounded. There is a bright, concentrated central bulge which fades gradually into the outer regions of the galaxy. The color gradient suggests a redder core, potentially indicating an older stellar population with relatively little ongoing star formation in the nuclear region. The outer regions exhibit a bluer hue, possibly indicating the presence of younger stars or low-level star formation. No distinct spiral arms or a prominent disk structure are discernible. There are no indications of major mergers or significant tidal disturbances affecting the overall structure of the galaxy. Faint extensions or irregularities are not apparent within the limitations of this image.
