The galaxy presents as an elliptical morphology, appearing largely featureless and smooth in texture. It displays a high degree of radial symmetry, tending toward a circular appearance. The light is concentrated towards the center, indicating a dense core or bulge with relatively little dust obscuration. Coloration indicates a significant population of older stars. There are no discernible spiral arms or bar structures. Overall the galaxy appears to be relatively isolated with no signs of major merger activity or tidal distortions.
