The galaxy presents as a centrally concentrated object, appearing largely smooth in structure with a slight elongation. There are no visible spiral arms or a prominent disk. The light distribution indicates a relatively uniform intensity across the galaxy's main body, gradually decreasing outwards. Its color is more reddish, with subtle variations in hue, possibly indicating an older stellar population. There may be some minor dust lanes or faint features, but they are not well defined. The galaxy appears relatively isolated, showing no signs of tidal interactions or ongoing merger activity.
