The galaxy presents a predominantly smooth morphology, with a high degree of central concentration. Its shape approximates a circular ellipse, showing minimal deviation towards a flattened or elongated structure. The color profile suggests an aging stellar population, indicated by a yellow hue. There may be evidence of a faint structure or disturbance within the galaxy, most notably a very small and faint patch or small spot near the galaxy. There is no indication of spiral arms, bar structures, or prominent dust lanes. The galaxy appears largely undisturbed, displaying no obvious signs of ongoing major mergers or interactions with other galaxies. It is likely a mature system.
