The galaxy appears as a centrally concentrated object with a generally smooth, featureless morphology. It exhibits a near circular shape. There are no discernible spiral arms or a prominent central bar, suggesting a lack of ordered rotation. The light distribution appears relatively even across the galaxy, with a gradual decrease in intensity from the core outwards. There are no obvious signs of recent or ongoing major merger activity, although subtle disturbances are not ruled out. Based on its observed characteristics, this galaxy appears to be a relatively quiescent system.
