The galaxy appears as a relatively smooth, elliptical structure with a dominant central bulge. The color profile suggests an older stellar population, with a yellowish-orange hue prevalent throughout. There is a slight asymmetry in the light distribution, potentially indicating a minor gravitational interaction or disturbance. There is a distinct, smaller, and redder component situated slightly to the right of the main body, which could be a satellite galaxy in the process of merging or a region of enhanced dust obscuration. The galaxy is relatively compact. Overall, the morphology indicates a relatively quiescent galaxy with possibly suppressed star formation.
