The galaxy appears to be elliptical in shape, with a smooth, concentrated light distribution. There is a distinct central bulge that dominates the overall structure. The galaxy's light profile fades gradually from the core outward, without any discernible spiral arm features or obvious dust lanes. The color suggests an older stellar population with a yellow-red hue, indicating a lack of significant recent star formation. The galaxy appears relatively undisturbed, showing no major signs of tidal interactions or ongoing mergers. The overall appearance suggests a relatively massive system.
