The galaxy appears to be an elliptical galaxy, exhibiting a smooth, concentrated morphology with an apparent lack of spiral arms or a prominent disk. Its central region is characterized by a bright, concentrated core, suggesting a significant concentration of stars. The color gradient shows a yellowish hue in the central regions, transitioning to bluer tones in the outer parts. This color difference might suggest a relatively older stellar population in the core. The galaxy's shape is approximately round. Overall, the galaxy appears relatively undisturbed, without any signs of major mergers or significant tidal distortions. Some minor irregularities could suggest possible weak interaction with smaller galaxies or past events. The overall structure suggests a well-evolved system with significant mass.
