The galaxy presents a generally smooth, elliptical morphology. It exhibits a central, high-intensity region that gradually decreases in brightness toward the outer edges. The color profile appears red-shifted, which suggests it is at a considerable cosmological distance. There is a hint of tidal disturbance or asymmetry visible, possibly indicating that the galaxy is the product of a past minor merger or interaction. The object's generally smooth appearance suggests that this object is most likely a galaxy, rather than other stellar objects. The galaxy's color implies an older stellar population with lower ongoing star formation.
