The galaxy presents as a centrally concentrated, luminous object. It appears primarily smooth in structure with a high degree of rotational symmetry. The overall morphology is largely spheroidal.  A subtle color gradient is observed, transitioning from a slightly bluer hue in the outer regions to a redder tone towards the core. There is no obvious evidence of spiral arms, a distinct disk, or significant tidal disturbances suggesting recent major merger activity. Faint, diffuse light extends outward from the core, gradually fading into the background sky. The lack of pronounced dust lanes further supports the categorization as a relatively unperturbed system.
