The galaxy presents as a relatively smooth, centrally concentrated object. Its morphology appears elliptical, with a high degree of radial symmetry. The color profile is predominantly yellow to red, suggesting an older stellar population and relatively low levels of ongoing star formation. There are no obvious spiral arm structures or dust lanes visible in this image. No active galactic nucleus is discernible within the limits of the image resolution. The galaxy exhibits no strong signs of recent major merger activity or tidal distortions. It appears to be a well-formed, early-type galaxy.
