The galaxy presents as a centrally concentrated elliptical system, appearing largely smooth in texture. Its core exhibits a bright, yellow-orange hue, suggesting a dominant population of older stars. As the radial distance increases from the core, the color transitions toward a more green/red distribution. The galaxy exhibits slight asymmetry, with the primary luminous structure being round, and the outermost region showing signs of a slight warp, indicating a potential past interaction or ongoing internal disturbance. Overall, the galaxy shows a classic elliptical morphology with signs of past or ongoing activity.
