The galaxy presents as a generally smooth, elliptical-like structure, though there is some indication of faint, diffuse features or a possible disk-like component within the broader halo. The shape appears generally round. There is no obvious sign of merging activity or strong tidal disturbance, though the presence of some minor internal asymmetries cannot be entirely ruled out. The galaxy's color is relatively uniform, trending toward redder wavelengths. This would imply an older stellar population and diminished current star formation. The galaxy has an estimated size on the order of several kiloparsecs. The data suggest this is a massive galaxy that has largely ceased star formation.
