The galaxy appears to be an elliptical type, characterized by a smooth, spheroidal morphology. There is a high concentration of light toward the center, with intensity gradually decreasing towards the edges. A slight elongation is present, but it appears generally round. The galaxy shows a predominantly yellow-red hue, suggesting a population of older stars and a relative paucity of ongoing star formation. The smooth light profile and color indices indicate that this is a fairly mature system with substantial mass. There appears to be a possible minor disturbance but it is unclear if this is the product of a small merger.
