The galaxy presents as a relatively smooth, elliptical-like object with a central, concentrated bulge. The light distribution indicates a generally spheroidal morphology. The color gradient suggests a population of older stars, particularly within the bulge, where light appears more yellow, transitioning toward slightly bluer hues in the outer regions. There is no distinct evidence of spiral arm structures or significant dust lanes. The overall appearance indicates a quiescent galaxy, possibly in a later stage of its evolution. Minimal visible disturbance suggests it has not experienced any recent major merger events.
