The galaxy appears to be a well-defined elliptical galaxy with a smooth, centrally concentrated light distribution. It exhibits a fairly regular, rounded shape with a high degree of symmetry. There is a lack of any prominent spiral arms or disk-like structures. The core is a bright yellow, indicating a population of older stars that have exhausted much of their hydrogen fuel, and little ongoing star formation. The galaxy appears relatively isolated, showing no obvious signs of recent major mergers or significant tidal disturbances in this image, though a very minor interaction cannot be completely ruled out. The overall color of the galaxy is skewed toward the redder end of the spectrum. This suggests an older stellar population. A slight gradient in color with increasing distance from the center can be observed, where the galaxy appears to be more red.