The galaxy presents as a somewhat centrally condensed object, its light profile appearing relatively smooth with no readily discernible spiral arm structures. The morphology leans towards elliptical, exhibiting a high degree of sphericity with a slight elongation. The core appears bright and compact, indicating a high concentration of stars and possibly a supermassive black hole. Overall, it looks to be quite massive. There's no evidence of any on-going major mergers or tidal disturbances from this image, suggesting it has likely experienced a relatively quiescent evolutionary history, although there might be some minor disturbances in the morphology. The overall color is fairly red, suggestive of an older stellar population and a low rate of star formation.
