The galaxy presents as a moderately bright, elliptical-shaped structure. Its core exhibits a high degree of luminosity, suggesting a significant concentration of stars within the central region. The light is somewhat redder, which suggests a population of older stars. Moving outward from the center, the galaxy's brightness diminishes gradually. There is no discernible spiral arm structure, and the overall form is relatively smooth and featureless. The galaxy does not appear to be undergoing any major mergers or significant tidal disturbances, with no obvious signs of asymmetry or extended tidal tails.
