This galaxy appears to be a relatively smooth elliptical galaxy, with a high degree of central concentration of light. It has a slightly elongated shape and a general reddish color, suggesting a population dominated by older stars. There is little evidence of spiral arms or significant dust lanes. The galaxy's profile appears undisturbed, exhibiting no obvious signs of recent major mergers, although a potential minor disturbance cannot be entirely ruled out. The overall structure indicates a relatively evolved system that may have undergone significant quenching of star formation.
