The galaxy appears as a centrally concentrated object, likely an elliptical or lenticular type. Its light profile seems smooth, lacking any distinct spiral arm structures. The central region exhibits a yellowish-orange hue, which may be indicative of an older stellar population and a lower rate of star formation. The outer regions transition to a greenish-blue color, possibly suggesting the presence of some younger, hotter stars, albeit at a lower overall proportion. There is a very faint hint of a disk shape, but overall the structure is largely spheroidal in appearance. No obvious signs of a major merger event are apparent, though some minor asymmetries or disturbances are possible.
