The galaxy appears as a centrally concentrated object with an overall elliptical morphology. It has a bright core that gradually fades into an extended, diffuse halo. The light distribution suggests a smooth profile, lacking prominent spiral arms or distinct features. The galaxy's color seems slightly redder than average, possibly indicating an older stellar population or a higher dust content. Its shape is elongated, though moderately so, with a fairly high degree of apparent flattening. There are no obvious signs of recent major merger events or significant tidal disturbances.
