The galaxy presents as an elliptical morphology, exhibiting a smooth, concentrated light distribution with minimal discernible internal structure. The light is more concentrated at the center and fades as it extends further out from the center. The color profile exhibits a yellowish-white hue, suggesting a stellar population dominated by older, lower-mass stars. There is a small area of blue hue on one side of the galaxy. The general shape of the galaxy is mostly round. There are no signs of spiral arms or prominent dust lanes and no major disturbances from merging activity.