The galaxy presents as a centrally concentrated, elliptical morphology, with a smooth light distribution suggesting a lack of significant spiral arm structure or prominent dust lanes. The core exhibits a bright, concentrated luminosity, fading gradually outwards towards the edges of the galaxy. Its color appears relatively uniform across the galaxy, indicating a population of older stars and potentially lower levels of ongoing star formation. There are no obvious signs of tidal disturbances or interactions with other galaxies, reinforcing its classification as a relatively undisturbed elliptical galaxy.
