The galaxy presents a relatively smooth, elliptical morphology. It displays a concentrated central bulge that dominates the overall light profile. The light gradually diminishes from the bright center. A subtle disk-like structure might be present, but any spiral arm features, if they exist, are faint and not easily discernible. The galaxy's shape is slightly elongated and it appears to have undergone minimal or no merging activity, based on the smooth, undisturbed light distribution. It exhibits a moderate redshift indicating it is a distant object, but not so distant that we cannot study its intrinsic light characteristics. The blue tinge observed in the image could be from younger, hotter stars, but the overall color suggests the galaxy is comprised predominantly of an older stellar population. The estimated mass seems consistent with a mid-sized galaxy. Low levels of star formation might be occurring, based on the spectral properties, but this is not apparent from visual inspection of the image.
