The galaxy presents as an elliptical or lenticular type, exhibiting a largely smooth morphology. There is a slight elongation with a moderate level of roundness. Evidence suggests it is a relatively massive system, with moderate levels of star formation. There is little indication of spiral arms or significant disk-like features. The galaxy appears mostly undisturbed, lacking signs of recent major mergers, though a minor disturbance is possible. The dominant color is moderately red, implying a relatively evolved stellar population and some dust content. Overall, the light profile suggests a centrally concentrated galaxy, consistent with an early-type classification at a considerable distance.
