The galaxy presents as a relatively smooth, elliptical-like structure with no apparent spiral arms or significant disk features. The central region displays a high degree of luminosity, suggesting a concentrated stellar population or active galactic nucleus. The light gradually fades from the center outwards, with the outer edges of the galaxy exhibiting a less defined, more diffuse appearance. There is a hint of reddish hue in the outer regions, possibly indicating an older stellar population, with more bluer stars near the center. No signs of any major mergers or tidal disturbances are obvious from the image. The overall morphology suggests an evolved galaxy, likely with a relatively low rate of star formation.
