The galaxy presents as a relatively smooth and centrally concentrated object. The overall morphology appears to be elliptical, exhibiting a gradual decline in surface brightness from the core outwards. The galaxy does not show any prominent spiral arm structures or distinct disk-like features. The light distribution indicates an even profile and there is no strong evidence of patchiness in the image, which may indicate very little star forming regions. Its color indicates a more mature stellar population. There is no observed tidal debris surrounding the system, nor any bright companions that would be suggestive of a merger event. 
