The galaxy presents as a central, moderately bright elliptical structure. There appears to be some slight bluing in color, suggesting a small amount of ongoing star formation. The galaxy appears to be fairly isolated with a small amount of interaction. It does not appear to be strongly interacting or undergoing a major merger event. The galaxy displays a concentrated, ellipsoidal morphology with no prominent spiral arms or bar structures visible. A small disturbance is present, suggesting a minor galactic event. The color gradients suggest a higher concentration of older stars toward the core. The overall shape is relatively smooth, without significant irregularities.
