This galaxy exhibits an elliptical morphology, appearing elongated with a smooth, diffused light distribution. The core region presents a yellowish hue, possibly indicating an older stellar population or dust obscuration. Moving outwards from the center, the galaxy fades into a bluish halo, suggesting the presence of younger, hotter stars potentially within a disk-like structure or tidal features. There are some signs of minor disturbances in the disk as it is likely not perfectly smooth. The observed ellipticity indicates a flattened spheroidal shape rather than a perfect sphere, showing a significant tilt relative to our line of sight. The gradual decrease in light intensity from the center outwards, coupled with the overall color gradients, points towards a galaxy with ongoing, but possibly decreasing, star formation activity.
