The galaxy appears as a singular, smooth object with a concentrated central region. Its color profile is slightly redder than the surrounding field, suggesting an older stellar population. The morphology is elliptical or spheroidal, lacking discernible spiral arms or prominent disk features. The object is generally uniform in appearance, displaying no significant disturbances or signs of ongoing merger activity. There is a notable radial gradient in luminosity, with the core being significantly brighter than the outer regions which quickly fade into the background. Its light is smooth and generally appears to be a mature galaxy with little to no star formation.
