The galaxy presents a relatively smooth, though not perfectly uniform, light distribution. It appears predominantly elliptical or spheroidal in shape, exhibiting a high degree of central concentration. The core is characterized by a bright, reddish-orange hue, suggesting a population of older stars and/or significant dust obscuration. There is a subtle indication of a possible tidal feature or minor disturbance in its structure, perhaps indicating a past interaction or ongoing merger event. The overall shape is generally round, with only a slight deviation towards an elongated form. Some evidence suggests a possible minor interaction or early stage merger, but the primary body of the galaxy remains relatively intact. The galaxy demonstrates a smooth overall appearance.
