The galaxy presents as a fairly smooth, elliptical-like structure with a concentrated central bulge. The core exhibits a yellowish hue, possibly indicating an older stellar population. Moving outward from the center, the light becomes more diffuse. There's a very slight suggestion of a flattened disk but the galaxy primarily appears spheroidal. No distinct spiral arms or bar features are discernible. The outer regions fade gradually into the background sky, suggesting a relatively smooth transition in stellar density. There is no strong evidence of significant tidal disturbances or ongoing merger activity in this image, though a minor disturbance can not be ruled out. Overall, this galaxy appears to be a relatively quiescent, evolved system.
