The galaxy presents a smooth, elliptical morphology, appearing largely featureless in this observation. Its color profile indicates an older stellar population, with a yellowish hue dominating the galaxy's core. The light distribution is concentrated towards the center, suggesting a dense nucleus. There may be some slight distortions or faint features indicating minor gravitational interactions, but the overall structure appears relatively undisturbed. The galaxy shows a low rate of star formation, further supporting the interpretation of a evolved stellar population. Its round shape implies a low angular momentum.
