The galaxy appears as a centrally concentrated object with a smooth, elliptical morphology. The light profile suggests a dominant bulge component. There is no prominent disk structure observed, although a subtle elongation is apparent, leaning towards a slightly oval shape. The galaxy exhibits a color gradient, with a bluer core and redder outskirts. No significant signs of tidal disturbances or ongoing mergers are visible; the galaxy appears relatively undisturbed. The overall luminosity indicates a massive system, with a high probability of being an early-type galaxy. There is no strong evidence of active star formation regions based on the smooth color distribution.
