The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits an elliptical morphology, appearing more spheroidal than disk-like. The color gradient suggests a central region that is yellower than the outer regions. The light distribution suggests a bulge-dominated system with minimal indications of spiral arm structure or significant dust lanes. There is a hint of a possible minor disturbance in its shape. The galaxy appears to be an isolated system, not part of a close interacting pair, though some asymmetry might hint at a past minor merger event.
