The galaxy appears as a single, relatively smooth object with a concentrated central region. It presents a golden hue, suggestive of an older stellar population dominating the light output. The morphological assessment indicates it is likely an elliptical galaxy with a primarily smooth structure, although at this resolution, finer details such as subtle disturbances or faint disk components may not be readily discernible. There appears to be a slight elongation, tending towards a round shape. The light distribution suggests a relaxed system, with no obvious signs of a recent major merger. The intense golden color indicates the presence of older stars, indicating that recent star formation is likely quite low.
