The galaxy appears to be a smooth, elliptical-type system, with a moderate ellipticity. There is some evidence of possible tidal disturbances or minor interactions. It exhibits a somewhat elongated morphology, deviating from a perfect circular shape. The color indices suggest the presence of both older stellar populations, with the presence of some on-going star formation. The lack of prominent spiral arms or strong dust lanes supports its classification as a relatively quiescent system. The galaxy's size is considerable. It seems to have experienced past interactions, although these events are not resulting in a full merging event at the current epoch.
