The galaxy presents as a single, largely unresolved object. Its morphology appears smooth and elliptical in shape with a high degree of roundness. There is no discernible disk structure, spiral arm features, or evidence of significant ongoing mergers or tidal disturbances. The object emits most strongly at redder wavelengths, and less intensely in bluer wavelengths. The size is compact, and it possesses a substantial mass. Its star formation rate appears low relative to its mass, suggesting a population dominated by older stars. The color profile implies a passively evolving system.
