The galaxy presents as a relatively smooth, elliptical structure. It exhibits a centrally concentrated luminosity profile, with a bright, yellowish core that gradually fades towards the outer edges. There is a slight elongation to the galaxy's shape, suggesting it is not perfectly spherical. The color distribution is relatively uniform, with subtle variations in hue, suggesting that it is largely comprised of older stellar populations. No distinct spiral arm structures or prominent dust lanes are apparent within the galaxy. There is no evidence of recent or significant merger activity within the galaxy's morphology.
