The galaxy presents as a centrally concentrated object with a smooth, relatively featureless morphology. It is approximately circular in shape, displaying a high degree of rotational symmetry. The light profile appears to decline gradually from the center, with no distinct spiral arms or bar structures visible. The color is slightly yellowish, suggestive of an older stellar population. There is no evidence of ongoing major mergers or significant tidal disturbances. The overall impression is that of a galaxy dominated by evolved stars, possibly an elliptical or S0 type galaxy at a considerable distance.
