The galaxy presents as a relatively compact and smooth object. Its morphology appears to be elliptical, exhibiting an elongated shape with a moderate axis ratio. The light distribution is centrally concentrated, with a bright core that gradually fades towards the outer regions. A faint stellar halo might be present, but this is difficult to determine with certainty due to the image resolution. There is no indication of any prominent spiral arm structure, bar, or ongoing major merger activity. The galaxy exhibits a redder color, suggesting an older stellar population and suppressed star formation. The smooth profile suggests a well-mixed stellar population, characteristic of evolved systems. Minor disturbances or tidal features are not readily apparent in this image.
