The galaxy presents a generally smooth and centralized morphology. The light distribution appears largely elliptical with a high degree of central concentration. There is very little apparent substructure. The overall color profile suggests a slightly redder hue, with some indication of a possible weak spiral arm structure. The object is somewhat elongated and displays a moderate degree of axisymmetry. The light appears to be relatively uniform across the galaxy's surface with no signs of tidal tails or obvious merger events currently in progress. There is a faint blue tint to the inner regions of the galaxy.
