The galaxy appears to be a relatively smooth, elliptical system. It exhibits a concentrated central bulge that dominates its overall structure. The light distribution transitions smoothly from a bright core to a fainter halo. There is no visible spiral arm structure or dust lanes apparent in the image. The galaxy displays a yellow-orange color, indicative of an older stellar population and lower levels of recent star formation. The morphology suggests that the galaxy is not currently undergoing any major merging events, although there might be minor distortions present.
