The galaxy presents as a relatively compact, centrally concentrated system. The overall morphology appears to be elliptical or lenticular, displaying a smooth, featureless profile with little to no discernible spiral arm structure or dust lanes. The light distribution is fairly uniform across the galaxy, with a gradual decline in intensity from the core outwards. The central region exhibits a somewhat brighter, more condensed core. Color gradients are subtle but suggest a redder, more evolved stellar population.
