The galaxy presents as a centrally concentrated object, with an elliptical morphology. The core region appears bright and relatively uniform in color, suggesting a population of older stars. Moving outward from the center, the light gradually diminishes, with a smooth transition to the galaxy's outer regions. There appears to be a slight bluer hue in the outer regions indicating younger stars are more prevalent. The galaxy appears largely undisturbed, showing no obvious signs of major mergers or tidal interactions.
