The galaxy appears to be a relatively smooth, elliptical system. Its overall color profile suggests a population of older stars, with a yellowish-orange hue dominating the central region. The light concentration is high towards the core, indicating a dense stellar population there. There is little to no visible evidence of spiral arms or prominent dust lanes. The galaxy is generally round, showing minimal elongation or distortion. There are no obvious signs of ongoing mergers or significant tidal disturbances in the immediate vicinity of the galaxy. Based on its color and morphology, the galaxy is likely an early-type system with a low star formation rate.
