The galaxy appears to be of moderate angular size. The overall light distribution suggests a primarily elliptical morphology, with a relatively smooth profile, though there are subtle indications of some possible features or substructure. The light is concentrated towards the center, gradually decreasing in intensity outwards. Color gradients are observed within the galaxy. The core appears redder, shifting to bluer tones in the outer regions, which indicates differing stellar populations or dust distribution. There is some evidence of minor disturbances and that it may be merging with a smaller object.
