The galaxy presents as a largely smooth, elliptical morphology. A bright, concentrated nucleus dominates the galaxy's luminosity profile. The main body exhibits a generally rounded shape. There is very little, if any, visual evidence of spiral arm structure or significant dust lanes. The galaxy appears to be a mature system, potentially with an older stellar population indicated by its color. There is a possible small tidal arm or galaxy to the south of the main galaxy body that may indicate some kind of disturbance or previous merging event.
