The galaxy presents as a single, centrally concentrated object with a smooth, relatively featureless morphology. The light profile appears to be consistent with an elliptical galaxy, exhibiting a radial decline in surface brightness from the core outward. The core region exhibits a yellowish hue, suggesting an older stellar population. The apparent lack of spiral arms or a prominent disk structure supports the classification as an elliptical. There is no discernible evidence of ongoing major merger activity or significant tidal disturbances. Faint, extended features are not apparent within the limitations of this image.
