The galaxy presents as a single, relatively smooth and centralized object. Its shape is generally elliptical, elongated with the appearance of a flattened spheroid. The central region exhibits a bright, concentrated core. The color is a mix of yellow, blue, and red hues which could be a result of varying stellar populations. The lack of obvious spiral arms or distinct features may indicate a relatively evolved state, dominated by older stellar populations, although some localized blue regions may indicate ongoing star formation. Based on visual inspection, the galaxy does not appear to be undergoing any major merger activity. There is some indication of possible minor disturbance or interaction, as it is not perfectly uniform in shape. 
