The galaxy appears as a single, relatively smooth and concentrated object. It presents with a predominantly elliptical morphology. There is minimal discernible internal structure beyond a gradual radial decrease in luminosity. The color profile suggests a relatively old stellar population, indicated by its yellow/red hue. There is no obvious spiral arm structure or significant dust lane obscuration. The overall appearance is consistent with an early-type galaxy that is not currently undergoing significant star formation activity. There may be some minor disturbances, but the appearance is largely undisturbed.
