The galaxy appears as a single, relatively smooth and rounded object. Its color is predominantly yellow-orange, possibly indicating an older stellar population. There is a clear, brighter core region dominating the overall structure. This central region is surrounded by a fainter, more diffuse halo or outer region. There is evidence of a possible minor interaction or internal disturbance. The galaxy does not present a strong spiral or barred structure and appears elliptical or lenticular in nature. There may be a larger galaxy in the process of merging as it has a double nucleus.
