The galaxy presents a largely smooth, elliptical morphology. The central region displays a concentrated luminosity, transitioning outward to a more diffuse halo. The color appears generally reddish-yellow, suggesting a stellar population dominated by older, redder stars, with a low ongoing star formation rate. The galaxy's shape appears close to round. There is no strong indication of a major ongoing merger, though subtle features suggest minor gravitational disturbances may be present.
