The galaxy presents a generally smooth, elliptical morphology. Its light profile appears relatively uniform, lacking prominent spiral arms or a well-defined central bulge. The overall color is yellowish-orange, suggesting a population of older stars with low rates of current star formation. There is a subtle hint of bluer regions towards the central area that may represent some amount of younger star formation. The galaxy's shape is moderately rounded, deviating only slightly from a perfect circle. There does not appear to be evidence of any major ongoing merger activity. The light distribution shows no pronounced tidal tails or other signs of significant gravitational disturbance, though there might be some minor distortion in the outer isophotes that could indicate a past interaction.
