The galaxy appears as a centrally concentrated object, exhibiting a relatively smooth morphology. There is no apparent spiral arm structure or a distinct bar feature. The light distribution indicates a possible elliptical or lenticular type galaxy. The object exhibits a somewhat round shape. A slight asymmetry in the outer regions is observed, perhaps indicating a minor gravitational disturbance or interaction with a smaller object. No obvious signs of a major merger event are visible. The galaxy's color is consistent with an older stellar population and relatively low ongoing star formation. The red-shift of the galaxy places it at a considerable distance.
