The galaxy presents a largely smooth, elliptical morphology. It exhibits a concentrated central bulge that appears roughly spherical.  There is a noticeable color gradient, with the core region appearing yellower than the outer regions. The galaxy appears to be relatively isolated with no major signs of recent or ongoing mergers or tidal disturbances. The outer regions exhibit a slight fading, suggesting a gradual decrease in stellar density with increasing distance from the center.  No distinct spiral arms or significant dust lanes are apparent in this image.
