The galaxy presents an overall elliptical morphology, appearing somewhat elongated with a slight tilt relative to the observer's line of sight. The light distribution suggests a concentration of older stars, evidenced by the reddish-yellow hue concentrated within the galaxy's central region. This central region appears smooth. There is a possible slight asymmetry or minor disturbance in the galaxy's structure, hinting at a possible past interaction or minor merger event, but it may simply be an artifact. Star formation seems to be occurring at a low rate.
