The galaxy presents as a moderately luminous object with a discernible elliptical morphology. The central region appears to be characterized by a relatively high surface brightness, suggestive of a concentrated stellar population. The isophotes are generally smooth, although there is a subtle indication of a possible weak disk or some kind of featured shape on the outer edges of the galaxy. The color profile seems to redden towards the center. The overall appearance suggests that the galaxy is not currently undergoing any major merger events or strong interactions.
