The galaxy appears as a moderately bright, elliptical-shaped object. Its light distribution is centrally concentrated, exhibiting a smooth, relatively featureless morphology. The color profile suggests a predominantly older stellar population, as indicated by its yellowish hue. The galaxy shows a slight elongation, deviating marginally from a perfect circular shape. There is no distinct spiral arm structure visible. The overall structure indicates that the galaxy does not show signs of major disturbances or ongoing mergers, with a possible minor companion object in close proximity. The galaxy displays a notable red shift indicating that this is an older galaxy.
