This galaxy presents a generally smooth morphology, with a notable concentration of light towards the center. The galaxy exhibits an elliptical shape and a noticeable lack of distinct spiral arm structures. The color profile suggests a dominant population of older stars, with a yellowish hue in the central region. The outer regions fade in intensity, displaying a redder color index, potentially indicating a decreasing density of younger, bluer stars in the periphery. The image suggests that this is a massive galaxy with a low rate of star formation. There are no signs of recent or ongoing major mergers or disturbances; the galaxy appears relatively undisturbed.
