This galaxy presents as a relatively smooth, centrally concentrated object with a nearly circular morphology. The light distribution suggests a dominant spheroid component. There is a hint of a disk but this is difficult to confirm with the level of detail in the image. The galaxy's color indices, derived from the DESI magnitudes, suggest a population of older stars, but there is also evidence of more recent star formation activity within the galaxy. There is a possible minor disturbance. It is also possible that this observation could be an artifact. There is no strong evidence for a major ongoing merger, nor for significant tidal features. The color profile also appears smooth, with no strong gradients or localized color variations, indicating a well-mixed stellar population or the dominance of a single population throughout the galaxy.
