The galaxy presents as a roughly elliptical structure with a high degree of central concentration. The light distribution appears smooth and featureless, lacking discernible spiral arms or bar structures. The color is primarily red-yellow, suggestive of an older stellar population with minimal ongoing star formation. The lack of blue light indicates a low abundance of young, hot stars. There is a slight elongation, hinting that it is neither perfectly circular nor a disk. There are no obvious signs of mergers or tidal disturbances, suggesting relative isolation or past mergers that have reached an advanced stage of dynamical relaxation. It appears to be a somewhat massive galaxy, with little to no current star formation activity.
