The galaxy presents as a centrally concentrated, elliptical morphology, with a smooth light distribution and minimal discernible substructure. The overall shape is generally round, though with a slight elongation. The core exhibits a bright, concentrated region, indicating a substantial population of older stars. The galaxy's color is relatively uniform, with a hint of redder hues, suggestive of an older stellar population and a low ongoing rate of star formation. There appears to be no evidence of strong tidal features or recent merger activity in the immediate vicinity of the galaxy. The light profile appears to gradually fade into the background, indicating an absence of a distinct edge.
