The galaxy presents an overall elliptical morphology, appearing relatively smooth with a concentrated central bulge. The bulge exhibits a yellow-white hue, suggesting an older stellar population dominated by evolved stars. The outer regions of the galaxy gradually fade into a diffuse halo. There's a subtle suggestion of a disk component, evidenced by a slight flattening of the galaxy's shape, though no distinct spiral arm structures are discernible. Irregularities or signs of major mergers are largely absent, though there is a slight disturbance visible. The galaxy's color gradients indicate some level of on-going star formation.