The galaxy presents as a centrally concentrated, smooth object with a generally elliptical morphology. The core region exhibits a bright, yellowish hue, suggesting a population of older stars. There is no apparent spiral structure or prominent dust lanes visible at this resolution. The outer regions of the galaxy appear fainter and redder, possibly indicating a decreasing density of stars or a population of older, redder stars. The galaxy does not exhibit any obvious signs of a major ongoing merger, although there is a faint hint of a minor disturbance in its symmetry. The overall appearance is consistent with that of an elliptical galaxy viewed at a moderate redshift. Based on the colors of the galaxy, it would appear that it is massive and has a low rate of star formation. 
