The galaxy presents as a fairly smooth, elliptical structure. It exhibits a central bulge that appears significantly brighter and more concentrated than the surrounding halo. The light distribution suggests a relatively high degree of radial symmetry, with a gradual decrease in luminosity from the core outward. The overall shape approximates a flattened spheroid, with the major axis oriented horizontally in the field of view. There is minimal evidence of spiral arm structure or significant dust lanes. The color profile indicates a dominant population of older stars, particularly in the bulge, with a redder hue compared to the slightly bluer, though still relatively old, stellar population in the outer regions. No signs of active galactic nuclei or strong starburst activity are immediately apparent from this image. The galaxy appears relatively isolated, showing no obvious signs of tidal interactions or ongoing mergers.
