The galaxy presents an elliptical morphology with a smooth, concentrated light profile. The core exhibits a bright, yellowish hue, which suggests an older stellar population and potentially a supermassive black hole. Moving outward from the core, the galaxy displays a gradual decrease in luminosity. The outer regions show a subtle flattening in shape, appearing slightly cigar-shaped. There is no discernible spiral structure or prominent dust lanes. The overall color is primarily yellow-red, consistent with evolved stars, but also slight traces of blue. There are no signs of major mergers or significant tidal disturbances. Faint, diffuse light extends beyond the main body of the galaxy, indicative of a halo of older stars.
