The galaxy presents as a relatively smooth, elliptical-like structure. The light distribution appears centrally concentrated with a gradual decrease in intensity outward. The galaxy exhibits a dominant yellowish-orange hue in its core, suggesting a population of older stars. There is very faint bluer light appearing at the edges of the galaxy. There is no discernible evidence of spiral arm structures or significant dust lanes. The galaxy appears undisturbed, lacking indications of recent mergers or major interactions.
