The galaxy presents as a primarily smooth, elliptical morphology. Its color profile indicates an older stellar population, with a dominant yellowish-red hue emanating from its core. There is no clear indication of significant disk structure or prominent spiral arms. A subtle deviation from perfect sphericity is observed, appearing slightly elongated. There are no signs of major ongoing mergers, although there might be faint indication of minor tidal disturbances. The light is highly concentrated, decreasing steadily from the center outward.