The galaxy presents as a generally smooth object, with a notable absence of spiral arms or a well-defined disk structure. The light is centrally concentrated, suggesting a bulge component. The overall shape appears somewhat rounded. There is a minor suggestion of asymmetry, possibly indicating a gravitational interaction or minor disturbance in the galaxy's structure. There is no clear evidence of an ongoing major merger event. Color analysis indicates a stronger signal in the green band compared to other regions of the spectrum. Overall the structure is most consistent with an elliptical or lenticular galaxy morphology, without obvious features. 
