The galaxy presents as a luminous, centrally concentrated object, with an overall elliptical morphology. The light distribution exhibits a smooth profile, suggesting a lack of prominent spiral arms or significant dust lanes. The core region is particularly bright, appearing yellow in color and gradually fading into more diffuse, redder outer regions. There is a slight elongation, but it appears predominantly round, with no obvious signs of recent merger activity or major tidal disturbances. The absence of distinct features points toward a relatively evolved system, potentially dominated by an older stellar population.
