The galaxy appears as a single, concentrated light source, generally elliptical in shape. Its light is fairly smooth and consistent in color without any obvious spiral arm structures or distinct features within. The galaxy's light is dominated by redder wavelengths, with only hints of bluer colors. This color profile implies a population dominated by older stars, possibly indicating lower current star formation. There is no visible sign of any ongoing interaction or disturbances that might change its regular shape. The color suggests a potentially high mass with low star forming activity.
