The galaxy appears to be an elliptical type. It exhibits a smooth, centrally concentrated light distribution with a gradual decrease in surface brightness extending outwards. The core of the galaxy appears bright and slightly blue, transitioning to redder hues in the outer regions. There is a subtle elongation, with an aspect ratio that deviates somewhat from perfectly circular. No distinct spiral arms or dust lanes are discernible. Indications are that there are no major mergers happening at this time. It appears to be a relatively isolated system with no prominent companion galaxies nearby.
