The galaxy presents a somewhat smooth, elliptical morphology, appearing largely spheroidal in shape. There is a subtle elongation, suggesting it is not perfectly circular. The central region exhibits higher luminosity, indicative of a concentrated stellar population or possibly an active galactic nucleus. There is a blue tinge to the galaxy, likely indicating recent star formation. There is some evidence of possible minor tidal disturbance on one side of the galaxy. This could be due to a past interaction with a smaller galaxy. The overall structure is relatively undisturbed, suggesting that if a merger occurred, it was either minor or happened long ago. The object is fairly compact and its size indicates that it is a relatively small galaxy.
