The galaxy presents as a centrally concentrated, elliptical structure with a smooth appearance. The core region exhibits a bright, yellowish-orange hue, suggesting a population of older stars. There's a subtle color gradient outward from the center, transitioning towards redder tones. The overall morphology indicates a relatively evolved system, likely with a high mass and low specific star formation rate. There are no obvious signs of spiral arms, dust lanes, or ongoing major mergers, though there may be a minor disturbance present. The galaxy appears to be largely undisturbed, with no prominent tidal features visible in the immediate vicinity.
