The galaxy appears to be a luminous, relatively smooth object. It exhibits a centrally concentrated structure, with the intensity of light gradually decreasing outwards from the core. The overall shape is elliptical, appearing largely round with a slight tendency towards a more elongated form. There are no distinct spiral arms or obvious signs of a prominent disk component visible in this image. Based on the color profile, the galaxy displays a reddish-yellow hue, suggesting a population of older stars. There are no indications of major ongoing mergers or significant tidal disturbances. 
