The galaxy presents a generally smooth morphology, with a high degree of central concentration. It exhibits an elliptical shape, appearing largely rounded with only a slight deviation from perfect circularity. The color profile suggests a relatively old stellar population, displaying a yellow-red hue. There is no visually discernible evidence of spiral arms, a central bar, or significant dust lanes. Furthermore, no obvious signs of major mergers or tidal disturbances are apparent in this image, although the possibility of minor interactions cannot be ruled out based solely on visual inspection.
