The galaxy appears to be a relatively smooth elliptical, exhibiting a high degree of central concentration. Its shape is generally round with only the slightest suggestion of elongation. There's no apparent spiral arm structure or prominent dust lanes visible. The light profile decreases steadily from the bright core outwards, and there is a very faint, extended halo surrounding the main body of the galaxy. There is no morphological evidence of ongoing major mergers or strong tidal disturbances, however, there may be some very faint indication of minor irregularities in the halo. The overall color appears somewhat redder, consistent with an older stellar population and suppressed star formation activity.
