The galaxy appears to be a relatively smooth, elliptical galaxy, exhibiting a concentrated central bulge and a diffuse halo. The core region displays a yellowish-orange hue, potentially indicative of an older stellar population dominated by redder giant stars. The outer regions gradually fade into a bluer shade, suggesting the presence of a younger stellar population or some degree of recent star formation, however limited. There is no apparent disk-like structure or spiral arms. The overall shape is largely round, with no major disturbances or signs of mergers visible in this image. The galaxy appears isolated and unperturbed, suggesting a relatively quiescent evolutionary history.
