The galaxy presents as a relatively smooth elliptical galaxy with a high degree of central concentration. The light profile appears to be uniformly distributed across the galaxy. No distinct spiral arm structures or bar features are discernible. The galaxy exhibits a slightly elongated shape. The color is predominantly reddish-yellow, suggesting a population of older stars. The image does not resolve individual stars or star clusters within the galaxy. There is no evidence of significant dust lanes or recent star formation activity. There may be a merger occurring with a dwarf galaxy, but the resolution makes it difficult to ascertain. 
