The galaxy presents as a largely featureless, elliptical-like morphology. Its central region exhibits a high concentration of luminosity, gradually decreasing toward the outer edges. The galaxy's color appears slightly redder, suggesting a population of older stars. There is no discernable spiral structure. The overall symmetry points towards a relaxed, dynamically stable system. No obvious signs of recent or ongoing major mergers or tidal disturbances are apparent in this image, however there appears to be a very slight hint of asymmetry to one side, so the possibility of minor interaction with another galaxy in the distant past cannot be ruled out. The relatively smooth appearance indicates that most of its stars are on random orbits, and there appears to be minimal ongoing star formation.
