This galaxy presents as a relatively smooth, elliptical structure. The core exhibits a bright, concentrated luminosity, with a color index that appears somewhat redder compared to the surrounding halo. The halo itself is less intensely illuminated and displays a bluer hue, suggesting the presence of a younger stellar population than that of the core. While the overall structure is largely featureless, there is a subtle indication of a slightly elongated shape. No spiral arms or bar structures are clearly discernible within the image, nor is there strong evidence of ongoing merging activity or significant tidal distortions.
