The galaxy presents as a centrally concentrated, smooth structure. It is a large galaxy. The light distribution is quite uniform, lacking distinct spiral arms or a prominent central bar. The overall shape appears close to round, with only a slight elongation discernible. The color appears to be a yellowish-orange hue, indicative of a stellar population dominated by older stars. There are no obvious signs of ongoing major mergers, although there may be slight disturbances in its structure suggesting minor gravitational interactions, or a past merger event. The surface brightness appears relatively even, with a gradual decrease in intensity from the center outwards. There is no strong evidence of significant recent star formation.
