The galaxy appears to be a relatively smooth, elliptical galaxy with a concentrated central bulge. It exhibits a yellowish-white hue, suggesting an older stellar population, with the lack of significant blue color indicating limited ongoing star formation. The galaxy displays a fairly circular morphology, with only subtle deviations from perfect roundness. There is no evidence of significant tidal disturbances, such as streams or shells, to suggest recent major merger activity, but this cannot be ruled out with the current image quality. The overall impression is that of a passively evolving galaxy, likely at a considerable cosmological distance.
