The galaxy appears to be a relatively large, luminous system, exhibiting an elliptical morphology. The core displays a concentrated, bright, yellow-orange hue, which could be indicative of an older stellar population dominating the central region. Moving outward from the core, the light transitions to a more diffuse, greenish-yellow color, suggesting the presence of younger stars or dust lanes. The overall shape is elongated, with a possible slight distortion on the left side of the galaxy. This suggests potential minor gravitational interactions or internal disturbances. The galaxy doesn't seem to exhibit any strong spiral arm structures and has a smooth appearance.
