The object appears to be a galaxy, likely an elliptical or lenticular type, exhibiting a smooth, centrally concentrated morphology. The galaxy displays a radial color gradient, transitioning from a brighter, yellowish core to a dimmer, slightly bluer outer halo. The isophotes appear generally regular, without significant signs of tidal disturbances or strong spiral arm structures. There is a faint suggestion of a flattened disk component embedded within the spheroid, but this is not definitive. The overall appearance suggests a relatively evolved stellar population, consistent with a low rate of ongoing star formation.
