The galaxy appears to be a relatively smooth, elliptical galaxy. It has a concentrated central bulge that emits primarily yellowish-white light, indicative of an older stellar population. There is a gradual decrease in luminosity moving outwards from the center. The outer regions of the galaxy are more diffuse, blending almost seamlessly into the background sky. There is no obvious disk structure or spiral arm features visible. It has a fairly circular shape, showing no signs of tidal disturbances or ongoing major mergers. There may be some very faint reddish structures in the periphery, that could indicate areas of some residual star formation. Overall, this galaxy presents as a mature, evolved system.
