The object appears as a single, relatively smooth galaxy, with a generally elliptical morphology. There is evidence of a potential minor disturbance on its left side, with a reddish tint, suggesting some level of ongoing or recent star formation in that region. The overall color gradient indicates a population of older stars dominating the main body of the galaxy, while a smaller region shows a younger, bluer stellar population. The galaxy exhibits a high degree of central concentration. While mostly smooth, subtle variations in color and brightness suggest internal substructure. There may also be interaction with a dwarf galaxy on the periphery. 
