The galaxy appears to be an elliptical type, characterized by a smooth, concentrated light distribution. It presents with a centrally concentrated bulge, showing a lack of spiral arm structure. There is no apparent dust lane or distinct features. Its overall shape is not perfectly spherical, appearing slightly elongated. There is no indication of any major merger activity; however, there seems to be some minor disturbances within the structure. The galaxy emits strongly across the g, r, and z bands, with brightness increasing from g to z band. The redder color suggests it is a relatively massive, evolved galaxy with lower ongoing star formation.
