The galaxy appears as a singular, concentrated object, exhibiting a smooth and generally round morphology. There is no apparent disk structure or spiral arm formation discernible in this image. The light profile appears centrally concentrated, with a gradual decrease in luminosity moving outwards from the core. The color suggests a population of older stars dominating the galaxy's composition, appearing more yellow/red in the spectrum, indicating lower levels of recent star formation. There is no significant sign of ongoing mergers or tidal disturbances.