The galaxy appears as a centrally concentrated object with a smooth, elliptical morphology. Its core exhibits a bright, yellowish-orange hue, suggesting a population of older stars. The light gradually fades as the radius increases. No spiral arms, distinct disk, or significant dust lanes are discernible. There are no signs of any major disturbances in the galaxy's overall structure or indications of ongoing merger events. The general color of the galaxy suggests minimal recent star formation.
