The galaxy presents an elliptical morphology, with a smooth light distribution lacking prominent spiral arms or a distinct bar structure. The core exhibits a concentrated, reddish hue, suggesting a population of older stars and possibly a significant dust component. The outer regions display a more diffuse, greenish color, potentially indicating ongoing, albeit subdued, star formation activity. There appears to be a minor disturbance in the overall symmetry, possibly from a past or ongoing minor merger event. The galaxy is relatively compact in apparent size, and it appears to have a mass of approximately 10^10 solar masses. The rate of star formation is low. The overall smoothness and color gradient suggest a relatively evolved system transitioning from a more active star-forming phase to a more quiescent state.
