The galaxy presents a largely smooth morphology, appearing somewhat rounded in shape. It exhibits a central concentration of light that gradually diffuses outwards. The color profile suggests a predominantly older stellar population, with a subtle blue hue possibly indicating some ongoing, but limited, star formation. There is no obvious spiral structure or bar visible. Some minor disturbances in its shape are noticeable. No clear signs of interaction with another galaxy or a major merger event are apparent, though some signs of minor disturbances exist in the galaxy's shape.
