The galaxy presents as a somewhat elongated, smooth object, with a high degree of central concentration. The core exhibits a yellow-orange hue, indicating a population of older stars. Moving outwards from the core, the color transitions to a less saturated, bluer white suggesting the presence of a younger stellar population in the outer regions. However, the galaxy appears primarily composed of older stars, given the dominant red-yellow color. There is a subtle asymmetry in the outer regions, suggesting a possible minor interaction or disturbance. Overall, the galaxy appears to be a relatively massive system. There are no signs of spiral arms or significant star formation, indicating an elliptical-like morphology.
