The galaxy appears to be a relatively smooth, elliptical or lenticular type. It exhibits a centrally concentrated brightness profile, with a gradual decrease in luminosity outwards. The object appears largely featureless, lacking prominent spiral arms or distinct dust lanes. Its shape is generally round. There is no obvious evidence of tidal tails or significant morphological disturbance indicative of a recent major merger event, although some minor disturbances cannot be ruled out. It shows a yellow/orange hue which could indicate an older stellar population and lower levels of recent star formation. The estimated size suggests this is a galaxy of moderate scale, and its absolute magnitude indicates that it is a relatively bright galaxy. Overall, this galaxy appears to be a relatively evolved system.
