The galaxy appears to be an elliptical, with a generally smooth, diffuse light distribution. The core region displays a concentrated brightness, suggesting a substantial central mass concentration. The overall shape appears relatively round, lacking any prominent spiral arm structures or significant tidal distortions. The galaxy's color suggests a moderately aged stellar population, exhibiting a blend of bluer and redder hues. The outer regions of the galaxy gradually fade into the background sky, indicating a lack of sharp edges or distinct boundaries. There are no immediately apparent signs of active galactic nuclei activity, intense star formation regions, or ongoing major mergers from visual inspection of the image.
