The galaxy presents as a relatively smooth, elliptical structure. The core exhibits a high degree of luminosity, appearing a yellow-orange hue, suggesting a population of older stars. The light intensity decreases gradually from the center outwards. There is minimal evidence of distinct spiral arms or prominent dust lanes. The shape is generally round, with only slight elongation observed. No obvious signs of major merging events are present. The overall color profile suggests a low star formation rate.
