The object appears to be a galaxy, exhibiting a generally smooth and elliptical morphology. The light profile is centrally concentrated, with a gradual decrease in intensity outwards from the core. The galaxy exhibits a warm color, suggesting an older stellar population and a relatively low rate of current star formation. There is no obvious spiral structure or dust lane visible in this image, lending support to the classification as an elliptical galaxy. The shape appears slightly elongated but mostly round with little disturbance. No merger activity is apparent in this image. 
